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Query : 2017A&A...605A..11M |
2017A&A...605A..11M - Astronomy and Astrophysics, volume 605A, 11-11 (2017/9-1)
Using binary statistics in Taurus-Auriga to distinguish between brown dwarf formation processes.
MARKS M., MARTIN E.L., BEJAR V.J.S., LODIEU N., KROUPA P., MANJAVACAS E., THIES I., REBOLO LOPEZ R. and VELASCO S.
Abstract (from CDS):
Abstract Copyright: © ESO, 2017
Journal keyword(s): binaries: general - stars: late-type - stars: low-mass - brown dwarfs - stars: formation - stars: formation
Simbad objects: 15
Number of rows : 15 |
N | Identifier | Otype |
ICRS (J2000) RA |
ICRS (J2000) DEC |
Mag U | Mag B | Mag V | Mag R | Mag I | Sp type |
#ref
1850 - 2024 |
#notes |
---|---|---|---|---|---|---|---|---|---|---|---|---|
1 | NGC 1333 | OpC | 03 29 11.3 | +31 18 36 | ~ | 1450 | 1 | |||||
2 | [PZR2014b] IC 348-SMM2E | Y*O | 03 43 57.73 | +32 03 10.1 | ~ | 24 | 0 | |||||
3 | IC 348 | OpC | 03 44 31.7 | +32 09 32 | ~ | 1392 | 1 | |||||
4 | Cl Melotte 22 | OpC | 03 46 24.2 | +24 06 50 | ~ | 3435 | 0 | |||||
5 | NAME Tau-Aur Complex | SFR | 04 30 | +25.0 | ~ | 1357 | 0 | |||||
6 | NAME Taurus Complex | SFR | 04 41.0 | +25 52 | ~ | 4416 | 0 | |||||
7 | NAME 25 Ori Group | OpC | 05 24 47.5 | +01 39 18 | ~ | 159 | 1 | |||||
8 | NAME Orion Nebula Cluster | OpC | 05 35.0 | -05 29 | ~ | 2331 | 0 | |||||
9 | Cl Collinder 69 | OpC | 05 35 10.1 | +09 48 47 | 2.8 | ~ | 313 | 0 | ||||
10 | NAME sig Ori Cluster | OpC | 05 38 42 | -02 36.0 | ~ | 567 | 0 | |||||
11 | NAME Cha 1 | MoC | 11 06 48 | -77 18.0 | ~ | 1154 | 1 | |||||
12 | OTS 44 | Y*O | 11 10 09.34392 | -76 32 17.8512 | M9.5+ | 60 | 0 | |||||
13 | Lupus 3 | SFR | 16 09.6 | -39 03 | ~ | 323 | 0 | |||||
14 | NAME Upper Sco Association | As* | 16 12 | -23.4 | ~ | 1369 | 1 | |||||
15 | NAME Ophiuchus Molecular Cloud | SFR | 16 28 06 | -24 32.5 | ~ | 3630 | 1 |
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