Brown dwarf candidates in the Serpens cloud core

Details Brown dwarf candidates in the Serpens cloud core Brown dwarf candidates in the Serpens cloud core

Jan 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006an....327...14e&link_type=abstract

Astronomische Nachrichten, Vol.327, Issue 1, p.14-16

Astronomy and Astrophysics

Astronomy

2

Stars: Formation, Stars: Low-Mass, Brown Dwarfs, Stars: Pre-Main Sequence, Infrared: Stars

Scientific paper

The Serpens cloud core is populated by a young, low-mass stellar cluster with members in many different evolutionary stages. We revisit the near-IR properties of the cluster in this contribution. A total of 188 near-IR sources are identified, including new members suggested in this work. Near-IR colour-magnitude and colour-colour diagrams allow us to suggest 42 objects among the cluster members as brown dwarf candidates. A considerable fraction of them present near-IR excesses which indicates that many of these very low mass objects are still surrounded by prominent dust accretion disks.
Workshop ``Ultralow-mass star formation and evolution'', see AN 326, No. 10

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