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Query : 2010ApJ...723..166D |
2010ApJ...723..166D - Astrophys. J., 723, 166-183 (2010/November-1)
A new method for the assessment of age and age spread of pre-main-sequence stars in young stellar associations of the Magellanic clouds.
DA RIO N., GOULIERMIS D.A. and GENNARO M.
Abstract (from CDS):
Abstract Copyright: ∼
Journal keyword(s): Hertzsprung-Russell and C-M diagrams - methods: statistical - open clusters and associations: individual: LH 95 - stars: formation - stars: pre-main sequence
Simbad objects: 8
Number of rows : 8 |
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 | NAME SMC | G | 00 52 38.0 | -72 48 01 | 2.79 | 2.2 | ~ | 11152 | 1 | |||
2 | NAME Magellanic Clouds | GrG | 03 00 | -71.0 | ~ | 7067 | 0 | |||||
3 | NGC 1748 | As* | 04 54 24.6 | -69 11 01 | 12.750 | 12.3 | ~ | 58 | 2 | |||
4 | NAME LMC | G | 05 23 34.6 | -69 45 22 | 0.4 | ~ | 17438 | 0 | ||||
5 | NAME Orion Nebula Cluster | OpC | 05 35.0 | -05 29 | ~ | 2332 | 0 | |||||
6 | NAME Ori Complex | Cld | 05 35.3 | -05 23 | ~ | 441 | 0 | |||||
7 | LHA 120-N 64C | EmO | 05 37 02.7 | -66 21 18 | ~ | 20 | 0 | |||||
8 | [HS66] 367 | As* | 05 37 03.767 | -66 22 02.69 | ~ | 47 | 0 |
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