Title of the table


You can sort by clicking on the column name.
Clicking a second time will reverse the sort.
Click on the refresh button to get the original version of the table.


Name HBC SFR Dist Ref Sep ('') Sep (AU) q ST Ref J H K L N EW(Ha) Ref. C? Notes
CoD -29     50 RZ93 0.500 25 1
M2e
M2
U+04
U+04
 
 
 
 
 
 
 
 
 
 
-2
 
DLR89
 
W
W
 
SZ128 607 LupIV 150 RZ93 0.600 90  
M1
M1?
B+96
HBC
 
 
 
 
 
 
 
 
 
 
-10
 
HBC
 
C?
W?
K-L et K-M (JLM juin 2004) show CW.
V853 Oph 266 Oph 140 RZ93 0.340 47.6  
M1.5
 
HBC
 
 
 
 
 
 
 
 
 
 
 
-41
 
HBC
 
C
C
q missing; CC based on KLM&N colors
WSB 3   Oph 140 RZ93 0.600 84  
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
W
W
WW based on colors
SR 9   Oph 140 RZ93 0.600 84 0.3
K5-K7
M4
GM01
GM01
 
 
 
 
 
 
 
 
 
 
-10.5
13.8
 
 
C
W
M4 from SED (GM01). if B=M4, should be W. Strange though. Variable ?
NTTS 162218-2420   Oph 140   0.190 26.6  
K5
 
 
 
 
 
 
 
8.29
8.53
8.22
8.58
 
 
 
 
 
 
W
W
WW based on colors. No resolved info hardly
Haro 1-4     140 RZ93 0.700 98 0.3
K5-6
 
CK79
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
C
W
CW based on colors (GM01); although N(B) is quite strong
Haro 6-10 389   140   0.500 70  
K3
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
C
C
Class I ; Br gamma in both comp H+95
WSB 11   Oph 140 RZ93 0.500 70  
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
?
?
K-N(AB)->both disks, but M. ?
HBC 360/HBC 361 360   140   7.200 1008 0.9
M3.5
M3
HK03
W+88
 
 
 
 
 
 
 
 
 
 
-6.7
-6.4
K+98
K+98
W
W
HBC360/361
SR 24 N 262 Oph 140   0.100 14  
M0.5
 
HBC
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
SR24N treated as a whole against SR24S
SR 24 S 262 Oph 140   5.100 714 0.35
K2
M0.5
HBC
HBC
 
 
 
 
 
 
 
 
 
 
-76, -71
-24, -74
HBC
HBC
C
C
Secondary Ha and Na EW's were from Wsb 42 listing in DB
SR 12 263 Oph 140   0.230 32.2  
M1-2
 
HBC
 
 
 
 
 
 
 
 
 
 
 
-4
 
HBC
 
W
W
WW from HBC as a whole + resolved colors
NTTS 155203-2338   Oph 140   0.600 84  
G3
 
HBC
 
 
 
 
 
7.21
8.65
6.69
8.57
 
 
 
 
 
 
W
W
WW from no Br-gamma (P+03) and KLM colors
RX J1535.8-2959   Usco-B 150   0.840 126  
M4
 
B+96
 
 
 
 
 
 
 
 
 
 
 
>-10
 
B+96
 
C
W
CW from B+96 and colors of components
HBC 634 634 Usco-A 150   0.203 30.45  
K0
 
W+99
 
8.48
10.17
7.84
9.62
7.71
9.27
 
 
 
 
-3.5
 
W+94
 
W
?
A=W from W+99 but nothing strong on B.
AS 353 A-Ba 292   150 T+04 5.700 855  
<M1, K2, K5
M2, M1.5
K2-BB90, K5 - R+05
(M1.5 - T+04)
10.03
10.22
9.16
9.2
8.23, 7.97
9.26
6.35, 6.24
8.7
 
 
-60, -124
-6, -4.4(Ba-Bb combined)
(-124, Ck79)
(4.4, Ck79)
C
C
Addl K, L from T+04, no Br gamma seen in either Ba-Bb.
AS 353 Ba-Bb     150 T+04 0.240 36  
M1.5
M1.5
T+04
T+04
 
 
 
 
9.26
9.45
8.7
9.32
 
 
 
 
 
 
C
W
CW based on K-L - no resolved line emission
HBC 275 AB 275   160 RZ93 5.000 800  
K7
M5
CK79
Ck79
 
 
 
 
 
 
 
 
 
 
-30, 27.8
-21, 18.5
(27.8, CK79)
(18.5, CK79)
C
C
Secondary is borderline WTTS.
HBC 275 AC 275   160 RZ93 0.830 132.8  
K7
?
CK79
 
 
 
 
 
 
 
 
 
 
 
-30, 27.8
 
(27.8, CK79)
 
C
?
Triple system identified by CCR95, PA similar to AB component
HBC 679 679   130 RZ93 4.500 585 #REF!
K5
M4, M3
P+03
(M3, P+03)
10.37
12.48
9.5
11.56
9.24
11.18
 
 
 
 
-0.2
-22
 
 
W
C
Where is Ha from? No brgamma in either component. JHK, spty, Av from P+03
Sz 108 620 Lupus 150 RZ93 4.200 630 #REF!
M0, M3
M4.5, M6
P+03, (M3 = CF+03)
P+03 (M6 = Cf+03)
9.76
12.02
9.09
11.21
8.78
10.86
 
 
 
 
-0.9, -0.5
-55,-53
(-0.5=HBC)
(-53=CF+03)
W
C
Photometry from P+03; br gamma emission seen in secondary, not primary. Where is Ha on primary from?
Sz 15     140 RZ93 10.600 1484 1
<M1
<M1
 
 
 
 
 
 
 
 
 
 
 
 
1.2
4.2
 
 
 
 
 
Sz 19 245 Cha 140 RZ93 4.600 644 #REF!
G2
M4
GM03
 
7.88
11.58
7.01
10.82
6.28
10.35
 
 
 
 
-20
-10
 
 
C
W
Resolved Photometry from WLK01. Where is resolved Ha from? CW designation based on Ha EW.
Sz 60   Cha II 200 RZ93 3.400 680 #REF!
M2, M1
M5, M4
(M1=HH92)
(M4=HH92)
11.59
11.55
10.49
10.6
9.83
10.08
 
 
 
 
-27, -17
-66, -94
(17=HH92)
(-94=HH92)
C
C
Resolved photometry, spTy and Ha from HH92
Sz 65 597   200 RZ93 6.500 1300 #REF!
<M1, M0, K7-M0 (HBC)
M5
(M0=H+94)
 
9.46
10.82
8.71
9.86
8.33
9.43
 
 
 
 
-5.9
-61
 
 
W
C
Resolved Photometry from WLK01. Where is resolved Ha from? WC designation based on Ha EW. M0, K7-M0 Spty are combined for AB compts.
Sz 68 248   150 RZ93 2.800 420 #REF!
K2
M5, M6
P+03
(M6=P+03)
7.67
10.58
6.96
9.78
6.62
9.29
6.07
8.81
 
 
-3.4
-16
 
 
W
W
Resolved photometry from GM01. P+03 - no brgamma detected in either component. Where is resolved Ha from? Note that primary used to be classified C, I reclassified W based on Ha.
(Sz 68)         0.100 0 #REF!
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
Sz 81 604 Lup II 150 RZ93 2.000 300 0.9
M5
M6
 
 
10.23
11.58
9.55
11.07
9.18
11.14
 
 
 
 
-59
-9
 
 
C
W
Resolved photometry from WLK01, H+94 - where is Ha and resolved spty from? CW based on Ha
Sz 88 612 Lup III 150 RZ93 1.500 225 0.3
M0
M4.5, M2
BZ97
(M2=BZ97)
9.97
11.71
9.14
10.38
8.6
10.59
8.03
10.45
 
 
-191, -130
-29, -34
(130=BZ97)
(34=BZ97)
C
C
Resolved photometry from GM01; Hband from WLK01. SpTy's differ! Changed from CW to CC based on Ha measurement alone.
WSB 28   oph 140 RZ93 5.000 700 #REF!
M2, M3
M7
(M3=P+03)
P+03 (M6 = Cf+03)
10.89
13.41
9.82
12.37
9.48
11.84
9.49
11.89
9.41
9.64
-4
 
 
 
W
 
Resolved photometry from P+03, L, N mag (really 8.8 micron) is from M+05. Where is Ha from?
WSB 4   oph 140 RZ93 2.800 392 #REF!
M4, M3
M3.5
(M3=P+03, M98)
P+03, M98)
11.7
11.55
10.96
10.69
10.63
10.12
9.5
9.21
 
 
-37, -29
-3, -4.4
(29=M98)
(4.4=M98)
C
W
L band looks very variable - cf P+03, M+05, and values given here .
WSB 71   oph 140 RZ93 3.400 476 #REF!
K2
M5, M6
P+03
(M6=P+03)
11
11.4
9.5
10.34
8.3
10
6.67
9.17
4.05
7.27
-37
-48
 
 
C
C
 
SZ Cha 566 Cha I 140 RZ93 5.200 728  
 
 
 
 
 
10.55
 
 
 
8.92
 
 
 
 
 
 
 
 
 
 
Unresolved spty=K0, with -8 Angs of EW(Ha) G-H02, -3.5 EWHa Reipurth et al. 1996
VW Cha AB 575 Cha I 160 W+97 0.661 105.76  
K5/K7
K7
BZ97
BZ97
9.21
10.87/9.83
8.05
8.96
7.25
9.32/8.89
 
 
 
 
79
48
 
 
C
C
There is a companion @ 17'' and the secondary is itself a 0.1" binary; system has Brgamma in emission (Gomez &Mardones2003); BZ97 get 48 Ang EWHa for 0.1" combined secondary
VW Cha BC   Cha I 160 W+97 0.100 16  
 
 
B+01, BZ97
 
10.55/9.83
 
8.96
 
8.92/8.89
9.75
 
 
 
 
 
 
 
 
 
 
K7 spty and 48 Ang EWHa is combined for 0.1" BC pair (BZ97)
CHXR 32   Cha I 140 RZ93 2.670 373.8  
K4/K3
G5
M+03, Chelli+88
Chelli+88
 
 
 
 
6.3
8.5
 
 
 
 
-
-9.3
 
Chelli+88
W
C
Secondary looks to be an IRC, although it is optically visible - interesting object to follow up
HD 97300   Cha I 190 P+97 0.840 159.6  
B9
 
G+97
 
7.7
 
7.4
 
7.3
10.3
 
 
 
 
 
 
 
 
 
 
No Li detected (Corporon & lagrange 1999) - star on ZAMS
C7-11   Cha I 140 RZ93 1.200 168  
K0-K3
 
Simbad, G-H02
 
 
 
 
 
8.98
9.1
 
 
 
 
 
 
 
 
 
 
G-H02 find unresolved EWHa=-3A (PDS 51)
Sz 41 588 Cha I 140 RZ93 1.900 266  
K0-K2
 
Simbad, G-H02
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
W
 
G-H02 find unresolved EWHa=-2A; is velocity variable (Reipurth+2002), is also very Ha variable (4.1 +- 16 A, Guenther & Emerson 1997)
LkHa 332-21 247 Cha I 140 RZ93 11.700 1638  
G8
 
Brooks+2001
 
 
 
 
 
 
 
 
 
 
 
-70.7
 
Reipurth+96
L+96
C
C
Secondary is CW Cha (SZ43) ; very wide binary
HM Anon   Cha I 140 RZ93 0.270 37.8  
G5
 
 
 
8.99
10.71
8.38
9.93
8.11
10.25
 
 
 
 
0.17(abs)
 
Walter1992
 
 
 
 
WX Cha 581 Cha I 160 G97 0.790 126.4  
K7/M0
 
GE97
 
10.22
11.84
9.2
11.01
8.43
10.94
 
 
 
 
-42.3+- 25
 
GE97
 
C
 
GE97 - variable Ha
HN Lup 601 Lup I 170 G+97 0.240 40.8  
M1.5
 
Simbad
 
9.9
10.1
8.57
9.07
7.76
8.71
 
 
 
 
 
 
 
 
 
 
Unresolved CTTS (Ha = -49.6, Nurnberger et al. 1997 A&A 324 1036); Spty for primary is unresolved spty for system
Sz 77 603 Lup I 170 G+97 1.800 306  
M0
 
Wichmann+99
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
Brgamma in absorption (GM03), unresolved Ha for system = -17.10 A (Wichmann+99) and -12.4 A (Nurnbergeret al. 1997)
Sz 91 614 Lup III 170 G+97 8.700 1479  
M0.5
 
Nurnberger+97
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
System Ha = 95.9 A (nurnberger et al. 1997)
HR 5999 619 Lup III 170 G+97 1.530 260.1  
A7eIII
 
Blondel+89
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
Variable Ha (double-peaked line) The et al. 1985 IrAJ, 17,79
Sz 105   Lup III 170 G+97 10.900 1853  
M4
 
Nurnberger+97
 
 
 
 
 
 
 
 
 
 
 
63.9
 
Nurnberger+97
 
C
 
Assuming secondary at ~11" doesn't contribute to Ha or spty
Sz 120   Lup III 170 G+97 2.700 459  
B3Vne
 
Simbad
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
Sz 123 629 Lup III 170 G+97 1.700 289  
M2
 
Simbad
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
S CrA 286 Cr A 130   1.410 183.3 #REF!
K3
M0
 
 
8.6
9.37
7.5
8.28
6.56
7.27
5.06
6.07
 
 
 
 
 
 
C
C
 
VV CrA 291 Cr A 130   2.100 273 #REF!
K4
 
R+05
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
C
C
 
LkHa 262 AB 8 and 9 MBM12 65 H+00 15.250 991.25 #REF!
M0
M3, M2, M4
L+01
L+01 (adopted), F+95 (M2), H+00 (M4)
 
 
 
 
9.66
9.52
8.84
8.97
7.02
7.07
-32.1
-25
H+00
L+01
C
C
Is a quadruple system. LkHa 262/Lkha 263ABC
LkHa 262 Ba-Bb 9 MBM12 65 H+00 0.410 26.65  
M3, M2, M4
 
L+01 (adopted), F+95 (M2), H+00 (M4)
 
 
 
 
 
9.52
 
8.97
 
7.07
 
-25
 
L+01
 
C
?
 
LkHa 262 Ba-Bc 9 MBM12 65 H+00 4.100 266.5  
M3, M2, M4
 
L+01 (adopted), F+95 (M2), H+00 (M4)
 
 
 
 
 
9.52
 
8.97
 
7.07
 
-25
 
L+01
 
C
?
 
J4872 AB   Tau 140   3.401 476.14 #REF!
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
Is a quadruple system - spty and photometry of A-B components (D+99, WG01) is contaminated with secondaries to A and B.
J4872 Aa-Ab   Tau 140   0.170 23.8 Duchene (1999)
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
FV Tau 386 Tau 140   0.704 98.56 0.85
K5
 
Hss94
 
 
 
 
 
7.92
8.37
7.31
7.03
4.07
4.92
-15/-6
-63/-41
(-6=WG01)
(-41=WG01)
C
C
 
UX Tau AB 43 Tau 140   5.860 820.4 0.5
K5
M2
WG01
WG01
 
 
 
 
7.5
8.98
6.74
8.89
5.62
8.31
-9.5
-4.5
WG01
WG01
C
W
 
UX Tau AC 43 Tau 140   2.630 368.2 0.15
K5
M5
WG01
WG01
 
 
 
 
7.5
10.57
6.74
10.19
5.62
10.06
-9.5
-8.5
WG01
WG01
C
W
 
DK Tau 45 Tau 140   2.304 322.56 #REF!
K9
M1
D+99
D+99
 
 
 
 
7.43
8.99
6.44
7.95
3.42
5.75
-31
-118
D+99
D+99
C
C
 
HK Tau 48 Tau 140   2.340 327.6 #REF!
M1
M2
D+99
D+99
 
 
 
 
8.68
12
7.86
11.54
5.28
8.46
-50
-12.5
D+99
D+99
C
C
 
Lk Ha 266 51 Tau 140   3.170 443.8 #REF!
M0.5
M2
WG01
WG01
 
 
 
 
8.76
8.49
8.32
8.18
5.44
8.21
-69
-7.2
WG01
WG01
C
W
 
GG Tau A 54 Tau 140   0.240 33.6 0.9
K7
M0.5
WG01
WG01
 
 
 
 
7.76
8.56
6.89
7.76
5.03
5.07
-57
-16
WG01
WG01
C
C
 
GG Tau B 54 Tau 140   1.400 196 0.3
M5.5
M7.5
WG01
WG01
 
 
 
 
10.11
12.02
9.3
11.23
6.72
8.8
-21
-32
WG01
WG01
C
C
 
UZ Tau A-Ba 52 Tau 140   3.600 504 0.9
M1
M2
WG01
WG01
 
 
 
 
7.56
8.7
6.69
7.83
3.50
6.43
-74
-54
WG01
 
C
C
Primary is also an SB so is a quadruple system
UZ Tau Ba-Bb     140   0.370 51.8 #REF!
M2
M3
WG01
 
 
 
 
 
8.7
9.3
7.83
8.63
6.43
6.6
-54
-97
 
 
C
C
Where is Ha and tertiary SpTy from ?
GK Tau 57 Tau 140   2.500 350 #REF!
K7
-
D+99
D+99
 
 
 
 
 
 
 
 
 
 
-35
-45
D+99
D+99
C
C
 
HN Tau 60 Tau 140   3.109 435.26 #REF!
K5
M4
WG01
WG01
 
 
 
 
8.01
11.73
6.6
11.14
 
 
-163
-87
WG01
WG01
C
C
 
IT Tau   Tau 140   2.400 336  
K3
M4
D+99
D+99
 
 
 
 
8.01
10.02
6.86
9.87
5.31
6.48
-21.7
-147
D+99
D+99
C
C
 
L1642-2 410 L1642 100   6.000 600  
K7
 
HBC
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
C
 
Ha detected by HBC but no EW measured
HBC 411 411 Tau 140   2.080 291.2  
 
 
 
 
 
 
 
 
 
 
7.86
9.8
4.68
7.21
 
 
 
 
 
 
No resolved Spty or Ha
L1642-1 413 L1642 100   2.700 270  
M
 
HBC
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
HV Tau AB-C 418 Tau 140   4.100 574  
M2
 
WG01
 
 
 
 
 
7.86
12.2
7.66
11.34
7.59
7.78
-4.3
-15
WG01
WG01
W
C
 
HV Tau AB     140   0.035 4.9  
M2
 
WG01
 
 
 
 
 
7.86
 
7.66
 
7.59
 
-4.3
 
WG01
 
W
W
 
Haro 6-37 Aa-Ab 73 Tau 140   0.330 46.2 0.8
 
 
 
 
 
 
 
 
 
 
 
 
5.04
5.47
 
 
 
 
 
 
 
Haro 6-37 AB 73 Tau 140   2.620 366.8  
K7
M1
WG01
 
 
 
 
 
 
 
 
 
4.48
4.68
-22
-184
 
WG01
C
C
Combined Aa-Ab has spty=K7, Ha=-22
RW Aur A-BC 80 Aur 140   1.410 197.4 0.7
K1
K5
WG01
WG01
 
 
 
 
7.06
8.64
5.94
7.92
3.12
5.96
-76
-43
WG01
WG01
C
C
Primary is also a SB so this is a quadruple system
RW Aur B-C 80 Aur 140   0.120 16.8  
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
CO Ori 84 Ori 500   2.000 1000  
F8
 
HBC
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
AR Ori 155 Ori 500   2.000 1000  
K7-M0
 
HBC
 
 
 
 
 
 
 
 
 
 
 
-29
 
CK79
 
C
 
 
LkHa 336 190       5.800 0  
K7-M0
 
 
 
 
 
 
 
 
 
 
 
 
 
-24
 
CK79
 
 
 
 
L1622-10     460   4.600 2116  
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
Pha 14 554   400 P87,R76 0.600 240  
M2
 
P87
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
C
 
 
Pha 30     400   0.700 280  
B2
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
VdBH 16     400   4.500 1800  
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
ESO Ha 280     400 RZ93 3.900 1560  
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
No ESO-HA 280 in SIMBAD ?
Pha 51 561       0.600 0  
K8
 
 
 
 
 
 
 
 
 
 
 
 
 
-70
 
P87
 
C
 
 
ESO Ha 29     400   4.200 1680  
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
PR94
 
W
 
Very weak Ha emission from PR94
HD 76534     400   2.100 840  
B2.5
 
V+00
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
Re 6         1.500 0  
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
Quite unknown object in Simbad
SX Cha 564   140   2.200 308 #REF!
M0.5
M3.5
Mu+05
Mu+05
 
 
 
 
 
 
 
 
 
 
-9.5
-8.9
Mu+05
Mu+05
W
 
Mu+05 inverted the SpT between components (mail from James M.)
ESO Ha 281         1.700 0  
M0.5
M4.5
 
BZ97
 
 
 
 
 
 
 
 
 
 
-1.1
-23
 
Bz97
W
C
BZ97 find Ha281(A) to be a background giant ??
VV Cha 573       1.100 0  
M1.5
M3
BZ97
BZ97
 
 
 
 
 
 
 
 
 
 
-94
-11
BZ97
 
C
W
 
Sz 30     140   4.500 630 #REF!
M0.5
M2
BZ97
BZ97
 
 
 
 
 
 
 
 
 
 
-11
-2.6
BZ97
BZ97
C
W
 
Hen 3-600   Hya 50   1.400 70 #REF!
M3
M3
GM01,DLR89
DLR89
 
 
 
 
 
 
 
 
 
 
-20
-8
DLR89
DLR89
C/W
W
Quite strong Ha (DLR89) but no real K-L excess on the prim. Variable ?
Sz 48         1.500 0  
K7
M0
BZ97
BZ97
 
 
 
 
 
 
 
 
 
 
-14
-39
BZ97
Bz97
C
C
 
BK Cha     200   0.780 156 1
K5/K7
M0.5
BZ97
BZ97
 
 
 
 
 
 
 
 
 
 
-54
-29
BZ97
Bz97
C
C
 
Sz 62         1.140 0  
M2
M3.5
BZ97
BZ97
 
 
 
 
 
 
 
 
 
 
-264
-70
BZ97
Bz97
C
C
 
Sz 119 627       0.590    
M2
M4
BZ97
BZ97
 
 
 
 
 
 
 
 
 
 
-4.1
-4.6
BZ97
Bz97
W
W
 
HER 4636     630 RZ93 3.900 2457  
B3
 
 
 
 
 
 
 
 
 
 
 
 
 
-26
 
GH+92
 
C
 
 
ESO Ha 283         2.100 0  
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
Sz 101         0.780 0  
M2.5
M3.5
BZ97
BZ97
 
 
 
 
 
 
 
 
 
 
-9.3
-44
BZ97
Bz97
W
C
 
Sz 116 625   150   1.500 225 #REF!
M1
M3
BZ97
BZ97
10.84
11.48
10.13
10.9
9.91
10.71
 
 
 
 
-4.1
-4.8
BZ97
Bz97
W
W
 
As 205 254   140   1.300 182 #REF!
K5
M3
PGS03
PGS03
8.15
9.24
7.16
7.97
5.9
6.9
4.9
5.8
 
 
-220
-55
 
 
C
C
 
WSB 18     140   1.040 145.6  
M2
M2.5
BZ97
BZ97
11.47
12.18
10.48
11.11
10.01
9.34
 
 
 
 
-8.4
-140
BZ97
Bz97
W
C
 
WSB 19     140   1.480 207.2 #REF!
M3
M5
BZ97
PGS03
11.16
11.76
10.13
10.85
9.53
10.38
 
 
 
 
-56
-37
BZ97
Bz97
C
C
 
WSB 26     140   1.100 154 #REF!
M0
M3
BZ97
BZ97
11.45
11.63
10.45
10.46
9.46
9.78
 
 
 
 
-109
-178
BZ97
Bz97
C
C
 
Elias 2-22 639 Oph 140   1.980 277.2 #REF!
K5
-
Doppman03
PGS03
9.2
9.2
7.8
7.8
7.13
8
6.42
6.15
 
 
 
 
 
 
C
C
Secondary is an IRC; brgamma detected in both components hence CTT/CTT designation
WSB 35   Oph 140   2.230 312.2 #REF!
M4
M6
PGS03
PGS03
11.17
11.83
9.98
10.98
9.17
10.56
8.28
10.25
 
 
 
 
 
 
C
W
CW based on brgamma detection/non-detection
Elias 2-26   Oph 140   1.400 196 #REF!
M3
M3
PGS03
PGS03
10.7
12.2
9.19
10.57
8.29
9.66
 
 
 
 
 
 
 
 
C
C
Variable brgamma emission seen - but both components seen to accrete on some occasions so went with CC
Elias 2-30   Oph 140   6.400 896  
G2.5
M4
PGS03
PGS03
8.77
12.03
7.45
10.54
6.4
9.7
5.25
9.26
 
 
 
 
 
 
W
W
Pgs03 see brgamma in abs in primary and non-detection in secondary
WSB 46 641/640 Oph 140 RZ93 10.300 1442  
M2
M5
Nurnberger+97
Nurnberger+97
 
 
 
 
 
 
 
 
 
 
-6.3
-3
Nurnberger+97
Nurnberger+97
W
W
 
Haro 1-14c-Haro1-14   Oph 140   12.900 1806  
K3
M0
Reipurth+2002
Reipurth+02
 
 
 
 
 
 
 
 
 
 
-
-45
Reipurth+02
CK79
W
C
Wide binary pairs WSB 69 with Haro 1-14c; haro 1-14c as a system is a WTTS according to lack of Ha
Haro 1-14c 644 Oph 140   0.011 1.5 0.31
K3
 
Reipurth+2002
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
SB (Simon & Prato 2004)
ROX 43   Oph 140   4.410 617.4  
G0
K5
BA92
BA92
 
 
 
 
6.66
7.74
5.51
7.22
 
 
-3.4
-0.8
BA92
BA92
 
W
 
Elias 2-49   Oph 140 Van den Ancker+97 1.130 158.2  
A2IVe
K4
Mora+01
BC01
6.99
9
6.18
8.14
5.32
7.73
 
 
 
 
-7.82
 
CR98
 
C
 
 
HBC 652 652       8.700 0  
K4
 
Simbad
 
 
 
 
 
7.55
 
7.32
 
 
 
 
 
 
 
 
 
 
ESO Ha 282   L162 160 RZ93 1.100 176  
 
 
 
 
9.8
11.1
8.6
10.1
7.8
9.5
6.8
8.6
 
 
 
 
 
 
C
C
Unresolved, EWHa = 54 angstroms (Gregorio-Hetem+92), J,H,K=9.82,8.61,7.88, class II SED. CC based on K-L colors
B59-1 AB   B59 160 RZ93 3.440 550.4  
 
 
 
 
 
13.1
 
11.5
 
11
 
10.2
 
 
 
 
 
 
 
C
Secondary CTTS based on K-L color
B59-1 Aa-Ab   B59 160 Koresko00 0.107 17.072  
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
B59-2 AB   B59 160 RZ93 3.110 497.6  
 
 
 
 
 
11.3
 
10.4
 
10.1
 
8.9
 
 
 
 
 
 
 
C
Secondary CTTS based on K-L color
B59-2 Aa-Ab   B59 160 Koresko00 0.012 1.952  
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
RNO 92 658 B62 225 RZ93 4.470 1005.75  
M0
 
 
 
 
 
 
 
 
 
 
 
 
 
-3.4
 
HBC
 
W
 
HBC has M0 with EWHa=3.4 A for combined system; given large separation we have assigned this to primary
V536 AQL 294   200 GM01 0.520 104  
K7
 
 
 
9.19
10.89
8.33
9.38
7.64
8.71
6.77
7.94
 
 
 
 
 
 
C
C
J-L photometry from GM01, CC based on K-L colors. K7 is unresolved spty and is assigned to primary. GM01 also list Ha for system of 52 A
IS Tau 59 Tau 140   0.220 30.8 #REF!
K7
M3.5, M4.5
WG01
M4.5=WG01
 
 
 
 
8.85
10.75
7.88
10.22
 
 
-9.5, -26
-24, -18
(-26=WG01)
-18=WG01
C
W
Don't know where -9.5/-24 Ha refs come from-JL?
FS Tau 383 Tau 140   0.230 32.2 #REF!
M0
M3.5
?
?
 
 
 
 
7.88
10
6.44
8.3
 
 
-71, -81
-33, -38
(-81=WG01)
-38=Wg01
C
C
What are refs for initial Ha and spty?
IW Tau 420 Tau 140   0.290 40.6  
 
 
 
 
 
 
 
 
9.05
9.16
8.99
8.82
 
 
 
 
 
 
 
 
Combined system has K7 spty and -4 Ang EWHa (Kenyon+98)
V410 Tau AB-C 29 Tau 140   0.290 40.6 #REF!
K4
M5.5
WG01
WG01
 
 
 
 
7.66
10.67
 
 
 
 
 
 
 
 
 
 
Combined Ha EW=-3 A (HBC), combined K-N for all 3 stars is 0.6 - class III. K4 is combined spty for AB
V410 Tau A-B 29 Tau 140   0.070 9.8  
 
 
 
 
 
 
 
 
7.77
10.17
 
 
 
 
 
 
 
 
 
 
 
V927 Tau   Tau 140   0.260 36.4 #REF!
M3
M3.5
HK03
HK03
 
 
 
 
9.23
9.76
7.82
8.76
 
 
-5.6
-2.5
HK03
HK03
W
W
 
V955 Tau   Tau 140   0.340 47.6 #REF!
K7
M2.5
HK03
HK03
 
 
 
 
 
 
 
 
 
 
-10.9
-6.2
HK03
HK03
C
W
 
V999 Tau   Tau 140   0.230 32.2 #REF!
M0.5
M2.5
HK03
HK03
 
 
 
 
 
 
 
 
 
 
-1.6
-4.5
HK03
HK03
W
W
 
V1026 Tau   Tau 140   0.660 92.4 #REF!
M2
M3.5
HK03
HK03
 
 
 
 
 
 
 
 
 
 
-57
-124
HK03
HK03
C
C
 
XZ Tau   Tau 140   0.310 43.4 #REF!
M2
M3.5
HK03
HK03
 
 
 
 
 
 
 
 
 
 
-77
-42
HK03
HK03
C
C
 
GH Tau   Tau 140   0.310 43.4 #REF!
M2
M2
HK03
HK03
 
 
 
 
 
 
 
 
 
 
-10
-10
HK03
HK03
C
C
 
GN Tau   Tau 140   0.330 46.2  
 
 
 
 
 
 
 
 
8.57
8.92
7.73
7.97
 
 
 
 
 
 
C
C
Combined spty=M2.5 (WB03) with Ha=-59 A, Aj=1.17 (luhman04). CC based on dereddened K-L colors
CZ Tau 31 Tau 140   0.320 44.8  
 
 
 
 
10.63
12.94
9.96
11.56
9.69
10.53
9.27
9.42
 
 
 
 
 
 
 
 
No known resolved spty or Ha measurements. Unresolved spty=M3, Ha=5.6 A.
V807 Tau   Tau 140   0.410 57.4 #REF!
K5
M2
HK03
HK03
 
 
 
 
 
 
 
 
 
 
-7.4
-3.4
HK03
HK03
C
W
 
LkCa 3   Tau 140   0.470 65.8  
 
 
 
 
 
 
 
 
8.06
8.24
8.02
8.19
 
 
 
 
 
 
W
W
WW based on K-L colors alone
DD Tau   Tau 140   0.568 79.52 #REF!
M3.5
M3.5
HK03
HK03
 
 
 
 
 
 
 
 
 
 
-206
-635
HK03
HK03
C
C
 
HBC 351 351 Tau 140   0.550 77  
 
 
 
 
 
 
 
 
9.2
10.6
 
 
 
 
 
 
 
 
 
 
 
HBC 412 412 Tau 140   0.700 98  
 
 
 
 
10.71
10.93
10.03
10.14
9.85
9.85
 
 
 
 
 
 
 
 
 
 
Combined SpTy=M2, Ha=-9 A (HBC), WTTS
VY Tau 68 Tau 140   0.660 92.4  
 
 
 
 
10.15
11.44
9.5
11.01
9.22
10.68
9.04
10.36
 
 
 
 
 
 
W
W
Combined SpTy=M0 (KH95); no Brgamma detected (GL96), EWHa=-4 A (HBC)
T Tau AB 35 Tau 140   0.695 97.3  
K0
IRC-featureless
WG01
Duchene+05
 
 
6.32
 
5.52
9.7
4.32
5.64
 
 
 
 
 
 
C
C
 
T Tau BC 35 Tau 140   0.118 16.52  
IRC-featureless
M1
Duchene+05
Duchene+05
 
 
>13.6
10.22
9.7
8.5
5.64
6.25
 
 
 
 
 
 
C
C
Based on resolved br gamma line EW from duchene+05, consistent with K-L colors
FV Tau/c   Tau 140   0.740 103.6 #REF!
M2.5
M3.5
HK03
HK03
 
 
 
 
 
 
 
 
 
 
-21
-800
HK03
HK03
C
C
 
FQ Tau   Tau 140   0.790 110.6 #REF!
M3
M3.5
HK03
HK03
 
 
 
 
 
 
 
 
 
 
-110
-23
HK03
HK03
C
C
 
UY Aur   Aur 140   0.880 123.2 #REF!
M0
M2.5
HK03
HK03
 
 
 
 
 
 
 
 
 
 
-36
-59
HK03
HK03
C
C
 
FX Tau   Tau 140   0.900 126 #REF!
M1
M4
 
 
 
 
 
 
 
 
7.65
8.65
 
 
-13
-1
 
 
C
W
 
LkCa 7   Tau 140   1.050 147 #REF!
M0
M3.5
HK03
HK03
 
 
 
 
 
 
 
 
 
 
-1.4
-2.2
HK03
HK03
W
W
 
HBC 358 358 Tau 199   1.580 314.42 #REF!
M3.5
M4
HK03
HK03
 
 
 
 
 
 
 
 
 
 
-4.5
-6.9
HK03
HK03
W
W
 
HBC 358A-359   Tau 140   20.100 2814  
M3.5
M2
HK03
Simbad
 
 
 
 
 
 
 
 
 
 
-4.5
-8.5
HK03
Martin+94
W
W
 
HBC 356/7 356 Tau 140   1.260 176.4  
K3
K3
 
 
 
 
 
 
10.72
10.77
10.86
10.92
 
 
-0.4
-0.4
 
 
W
W
 
HBC 354/5 354 Tau 140   6.300 882  
K0
K2
 
 
 
 
 
 
10.15
10.99
10.16
11.03
 
 
-1.2, +4.7
-1.2, +1.8
HSS94, 4.7 in abs Martin+94
+1.8 Martin+94
W
W
 
NTTS 155913-2233 AB-C   Usco     0.300 0  
 
 
 
 
 
 
 
 
8.49
9.33
 
 
 
 
 
 
 
 
 
 
AB is a 2.4 d period SB (Prato+02). Unresolved spty=K5, EWHa=-0.6 A (Martin98)
ROX 31 642 Oph 140   0.380 53.2  
 
 
 
 
 
 
 
 
8.68
8.97
8.31
8.85
 
 
 
 
 
 
W
W
K7 unresolved spty with Ha=-3.3 A (Ba92); WW based on dereddened K-L colors
DoAr 51 647 Oph 140   0.750 105  
 
 
 
 
 
 
 
 
7.75
10.22
7.86
9.19
 
 
 
 
 
 
W
C
K2, EWHa=-9.2 A unresolved (BA92); WC based on K-L colors
YLW 15A-GY263   L1688 140   7.600 1064  
K5
 
GL02
 
 
 
14.2
15.7
9.72
12.69
6.7
11
 
 
 
 
 
 
C
C
A class I source paired with a class II object. Brgamma seen in emission in primary, no decent SNR on secondary
YLW 15A   L1688 140 Girart+04 0.590 82.6  
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
DF Tau   Tau 140   0.099 13.86 #REF!
M2
M2.5
HK03
HK03
 
 
 
 
 
 
 
 
 
 
-55
-52
HK03
HK03
C
C
 
FO Tau   Tau 140   0.146 20.44 #REF!
M3.5
M3.5
HK03
HK03
 
 
 
 
 
 
 
 
 
 
-137
-95
HK03
HK03
C
C
 
NTTS 155427-2346   Sco-Cen 145   1.324 191.98  
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
Martin98 combined Spty=M0.5, EWHa=-0.9, WTTS
NTTS 160328-1921   Sco-Cen 145   0.578 83.81  
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
Martin98 combined SpTy=M0.5, EWHa=-19.3,CTTS:
NTTS 160735-1857   Sco-Cen 145   0.299 43.355  
 
 
 
 
10.27
10.73
9.48
10.06
9.29
9.71
 
 
 
 
 
 
 
 
 
 
Martin98 combined SpTy=M3, EWHa=-2.9, WTTS
NTTS 160905-1859 AB 633 Sco-Cen 145   3.429 497.205  
K0
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
Martin98 combined SpTy=K0, EWHa=0.3 (abs), WTTS; K-L =0.16 (Maserotti+05)
NTTS 160905-1859 Aa-Ab   Sco-Cen 145   0.0006 0.0932 0.18
K0
M4
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
An SB - spty are from best correlations in 2D correlation (Prato+02)
NTTS 155219-2314   Sco-Cen 145 Kohler+00 1.485 215.325  
 
 
 
 
10.66
11.58
9.94
11.02
9.69
10.78
 
 
 
 
 
 
 
 
 
 
Martin98 combined SpTy=M2.5, EWHa=-13.3, PTTS
NTTS 155331-2340   Sco-Cen 145 Kohler+00 0.092 13.34  
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
Martin98 combined Spty=M1.5, EWHa=-1.4, PTTS:
NTTS155808-2219   Sco-Cen 145 Kohler+00 0.193 27.985  
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
Martin98 combined SpTy=M3, EWHa=-3.3, WTTS:
NTTS 160248-1956   Sco-Cen 145 Kohler+00 0.643 93.235  
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
Martin98 combined SpTy=M2, EWHa=-4.0, PTTS:
NTTS 160728-1856 AB   Sco-Cen 145 Kohler+00 4.604 667.58  
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
Martin98 combined SpTy=M1, EWHa=-3.8, PTTS:
NTTS 160728-1856 BC   Sco-Cen 145 Kohler+00 4.201 609.145  
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
RZ93 = Reipurth & Zinecker 1993, A&A, 278, 81
U+04 = Uchida et al., 2004, ApJSS, 154, 439
DLR89 = De la Reza et al., 1989, ApJ 343, L61
GM01 = Geoffray & Monin, 2001, A&A369, 239
B+96 = Brandner et al., 1996, A&A 307,121
CK79 = Cohen & Kuhi 1979
H+95 = Herbst et al. 1995, ApJ 444
K+98 = Kenyon et al., 1998, AJ 115, 2491
HK03 = Hartigan & Kenyon, 2003, ApJ, 583, 334
W+88 = Walter et al., 1988, AJ 96, 297
P+03 = Prato et al., 2003, ApJ 584
W+94 = Walter et al., AJ 107, 692
BB90 = Basri & Batalha 1990, ApJ, 363, 654
T+04 = Tokunaga et al. 2004, AJ 127, 444
CCR95=Chelli, Cruz-Gonzalez & Reipurth 1995, A&AS, 114, 135
CF+03 = Comeron, Fernandez et al. 2003, A&A, 406, 1001
GM03=Gomez & mardones 2003, AJ, 125, 2134
WLK01 = Woitas, Leinert & Kohler 2001, A&A, 376, 782
HH92=Hughes & Hartigan 1992, AJ, 104, 680
H+94 = Hughes et al. 1994, AJ 108 107
M+05 = McCabe et al. 2005 ApJ submitted
M98=Martin, 1998, AJ, 115, 351
R+05 = Rice et al. 2005 in prep
H+00 = Hearty et al. 2000 A&A 353, 1044
L+01 = Luhman, K.L., 2001, ApJ, 560, 287
F+95=Fernandez et al. 1995, A&AS 114 439
WG01=White & Ghez 2001 ApJ 556, 265
D+99 =Duchene, Monin, Bouvier & Menard, 1999, A&A, 351, 954
HSS94=Hartigan, Strom & Strom 1994, ApJ, 427, 961
BZ97=Brandner & Zinnecker 1997
Chelli+88=Chelli et al. 1998, A&A, 207, 46
Walter, F., 1992, AJ, 104, 758
GE97=Guenther & emerson 1997, A&A, 321 803
G+97= Ghez et al. 1997
Wichmann+99 = Wichamnn et al. 1999 MNRAS, 307, 909
Blondel+89=Blondel et al. 1989, A&ASS, 80, 115
Doppman03=Doppmann, Jaffe, White 2003, AJ, 126, 3043
Reipurth+2002=Reipurth et al. 2002, AJ, 124, 2813
BA92=Bouvier & Appenzeller 1992, A&AS 92 481
Kouwenhoven+05=Kowenhouven et al. 2005 A&A 430 137
Mora+01=Mora et al. 2001 A&A 378, 116
Van den Ancker+97=van den Ancker et al. 1997 A&A 324, L33
BC01=Bouvier & Corporon 2001
CR98=Corcoran & Ray 1998 A&A 331 147
GH+92=Gregorio-Hetem+92=Gregorio-Hetem et al. 1992, AJ, 103, 549
WB03=White & Basri 2003, AJ, 582, 1109
luhman04=Luhman, 2004, ApJ, 617, 1216
GL96=Greene & lada 1996, AJ, 112, 2184
Duchene+05=Duchene, Ghez, McCabe & Ceccerelli 2005, ApJ, 628, 832
Prato+02=Prato et al. 2002, ApJ, 569, 863
Martin98=Martin, 1998, AJ, 115, 351
Girart+04=Girart et al. 2004, AJ, 127, 2969
Kohler+00=Kohler, Kunkel, Leinert & zinnecker 2000 A&A 356, 541
Chavarria+00=Chavarria, Terrenegra, Moreno-Corral & De Lara, 2000 A&AS, 145, 187
P87=Pettersson, 1987, A&A 171, 101
R76=Reynolds, 1976, AJ 206, 679
PR94=Pettersson & Reipurth, 1994, A&AS 104, 233
V+00=Valenti et al. 2000, ApJS 129, 399
Mu+05=Muzerolle et al. 2005, ApJ 625, 912
H+98=Hartmann et al. 1998, ApJ 495, 385
L+96=Lawson et al., 1996, MNRAS 280, 1071
Last modified: Sun Jan 22 16:56:15 US Mountain Standard Time 2006