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Very Low Mass Stars and Brown Dwarf Candidates in Orion OB1a and OB1b
Published online by Cambridge University Press: 26 May 2016
Abstract
VRI images within the belt of Orion and the Ori OB1a association reveal a pre-main sequence locus extending to below our completeness limit of about V=21. We report here on followup JHK imaging and optical and near–IR spectroscopy of the faintest and reddest of the PMS candidates. We find that they are unreddened mid-to-late M “stars” which fall on a few million year isochrone. Masses are largely substellar, reaching as low as about 0.02 M⊙ (20 Jovian masses). The space density of the substellar objects is high.
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- Part 2. Observations of Recently Born Substellar Objects
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- Copyright © Astronomical Society of the Pacific 2001