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The formation of a star cluster: predicting the properties of stars and brown dwarfsYoung massive stars in the ISOGAL survey. II. The catalogue of bright YSO candidatesPhotometric variability of young brown dwarfs in the $\mathsf{\sigma}$ Orionis open clusterPhotometric variability of a young, low-mass brown dwarfTheσ Orionis substellar population
P2860
description
article publié dans la revue scientifique Astrophysical Journal
@fr
im Juni 2002 veröffentlichter wissenschaftlicher Artikel
@de
scientific article published in the Astrophysical Journal
@en
wetenschappelijk artikel
@nl
наукова стаття, опублікована в червні 2002
@uk
name
A Young Very Low Mass Object Surrounded by Warm Dust
@en
A Young Very Low Mass Object Surrounded by Warm Dust
@nl
type
label
A Young Very Low Mass Object Surrounded by Warm Dust
@en
A Young Very Low Mass Object Surrounded by Warm Dust
@nl
prefLabel
A Young Very Low Mass Object Surrounded by Warm Dust
@en
A Young Very Low Mass Object Surrounded by Warm Dust
@nl
P2093
P50
P356
P1476
A Young Very Low Mass Object Surrounded by Warm Dust
@en
P2093
P304
P356
10.1086/341361
P407
P577
2002-06-01T00:00:00Z
P818
astro-ph/0204472
P819
2002ApJ...571L.155T