Spectroscopy of putative brown dwarfs in Taurus

K. L. Luhman, E. E. Mamajek

Research output: Contribution to journalArticle

8 Scopus citations

Abstract

Quanz and coworkers have reported the discovery of the coolest known member of the Taurus star-forming complex (L20.5), and Barrado and coworkers have identified a possible protostellar binary brown dwarf in the same region. We have performed infrared spectroscopy on the former and the brighter component of the latter to verify their substellar nature. The resulting spectra do not exhibit the strong steam absorption bands that are expected for cool objects, demonstrating that they are not young brown dwarfs. The optical magnitudes and colors for these sources are also indicative of background stars rather than members of Taurus. Although the fainter component of the candidate protostellar binary lacks spectroscopy, we conclude that it is a galaxy rather than a substellar member of Taurus based on its colors and the constraints on its proper motion.

Original languageEnglish (US)
Pages (from-to)L120-L124
JournalAstrophysical Journal Letters
Volume716
Issue number2 PART 2
DOIs
StatePublished - 2010

All Science Journal Classification (ASJC) codes

  • Astronomy and Astrophysics
  • Space and Planetary Science

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