Table 1
Observed objects in Chamaeleon.
Objecta | RA | Dec | System | Bin. | Spectral- | SpT | Dist. | Dist. | 2MASS | Backg.e |
[h m s]a,b | [° ′ ′′]a,b | architecturec | Ref. | types | Ref. | [pc] | Ref. | K [mag]d | density | |
|
||||||||||
RX J0915.5-7609 | 09 15 29.12 | –76 08 47.2 | ** | 1 | K7+? | 2 | 168 | 3 | 8.488 | 0.135 |
RX J0919.4-7738 | 09 19 24.96 | –77 38 37.0 | SB2+** | 4, 2, 1 | G7+?+K0+? | 5 | 57 | 6 | 6.780 | 0.137 |
RX J0935.0-7804 | 09 34 56.04 | –78 04 19.4 | ** | 1 | M2+? | 2 | 168 | 3 | 8.889 | 0.132 |
RX J0952.7-7933 | 09 53 13.74 | –79 33 28.5 | *+SB2 | 2, 1 | F6?+F6+F6? | 2 | 170? | 7 | 7.994 | 0.122 |
RX J1014.2-7636 | 10 14 08.07 | –76 36 32.8 | ** | 1 | M3+? | 2 | 165? | 8.874 | 0.154 | |
SZ Cha | 10 58 16.77 | –77 17 17.1 | SB?+*+w* | 8, 9 | K0+M5+? | 9, 10 | 165 | Cha I | 7.758 | 0.144 |
Ced 110 IRS 2 | 11 06 15.41 | –77 21 57.0 | **+w* | 10, 11 | G5+?+? | 12 | 165 | Cha I | 6.419 | 0.056 |
Cha Hα 2 | 11 07 42.46 | –77 33 59.4 | ** | 13, 14 | M6+M6? | 15 | 165 | Cha I | 10.675 | 0.062 |
VW Cha | 11 08 01.49 | –77 42 28.9 | SB?+**+w* | 16, 17 | K6+K7+?+M2.5 | 18 | 165 | Cha I | 6.962 | 0.088 |
RX J1109.4-7627 | 11 09 17.70 | –76 27 57.8 | ** | 19, 20 | K7+? | 2 | 165 | Cha I | 8.701 | 0.141 |
HD 97300 | 11 09 50.02 | –76 36 47.7 | ** | 8 | B9+? | 21 | 179 | 6 | 7.149 | 0.098 |
WX Cha | 11 09 58.74 | –77 37 08.9 | ** | 8 | K0-M1.25+? | 12 | 165 | Cha I | 7.970 | 0.096 |
WY Cha | 11 10 07.05 | –76 29 37.7 | **+w* | 20, 10 | K2-M0+?+? | 12 | 165 | Cha I | 8.451 | 0.127 |
HJM C 7-11 | 11 10 38.02 | –77 32 39.9 | SB?+*+w* | 8, 22 | K3+?+? | 2 | 165 | Cha I | 8.277 | 0.107 |
Sz 41 | 11 12 24.42 | –76 37 06.4 | SB?+*+w* | 23 | K4+?+G8 | 2, 24 | 165 | Cha I | 7.999 | 0.166 |
HM Anon | 11 12 42.69 | –77 22 23.1 | ** | 8 | G8+? | 25 | 165 | Cha I | 7.880 | 0.124 |
Notes.
Taken from the SIMBAD database (Wenger et al. 2007).
Previously known and supposed multiplicity of the objects: *: star, **: binary, SB: spectroscopic binary, SB2: double-lined spectroscopic binary, w*: wide stellar companion candidate.
References. (1) Köhler (2001). (2) Covino et al. (1997). (3) Sartori et al. (2003). (4) Torres (1986). (5) Torres et al. (2006). (6) van Leeuwen (2007). (7) Frink et al. (1998). (8) Ghez et al. (1997). (9) Reipurth et al. (2002). (10) Kraus & Hillenbrand (2007). (11) Simultaneously imaged. by Lafrenière et al. (2008) and by us (here). (12) Luhman (2007). (13) supposed by Neuhäuser et al. (2002). (14) confirmed by Ahmic et al. (2007), Lafrenière et al. (2008) and Schmidt et al. (2008b). (15) Schmidt et al. (2008b). (16) wide companion candidate: Reipurth & Zinnecker (1993), close binary: Brandner (1992), close triple: Brandeker et al. (2001). (17) Possibly SB in Melo (2003) and Torres et al. (2006), but could be the signal of the close triple. (18) Brandner & Zinnecker (1997), Sz 23 (VW Cha D?): Comerón et al. (1999). (19) Damjanov et al. (2007). (20) Lafrenière et al. (2008). (21) Rydgren (1980). (22) SB?: Torres et al. (2006), w*: Kraus & Hillenbrand (2007). (23) **, w*: Brandner (1992); Reipurth & Zinnecker (1993), SB? (primary and secondary in spectrograph entrance window): Reipurth et al. (2002). (24) Hyland et al. (1982). (25) Preibisch (1997).
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