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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