Very Low Mass Objects in Orion OB1a and b

Details Very Low Mass Objects in Orion OB1a and b Very Low Mass Objects in Orion OB1a and b

Feb 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009aipc.1094..568w&link_type=abstract

COOL STARS, STELLAR SYSTEMS AND THE SUN: Proceedings of the 15th Cambridge Workshop on Cool Stars, Stellar Systems and the Sun.

Computer Science

Databases

Low Luminosity Stars, Subdwarfs, And Brown Dwarfs, Astronomical Catalogs, Atlases, Sky Surveys, Databases, Retrieval Systems, Archives, Etc., Star Formation

Scientific paper

We present initial results of a search for the substellar mass population of the Orion OB1 a and b associations, based on a deep optical/near-IR survey. We are complete to about 1 magnitude fainter than the 2MASS survey at K. Global comparison of the K vs. J-K color-magnitude diagram shows an excess of objects with K>14.4 (the substellar limit in Orion OB1b) and 0.8

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