Possible substellar objects in the RHO Ophiuchi cloud

Research output: Contribution to journalArticle

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Abstract

Three sources have been discovered in the embedded population of the ρ Ophiuchi cloud that have dereddened MK ≥ 7. Comparison with theoretical models for evolution of low-mass stars shows that these sources are substantially less luminous than expected for objects evolving onto the main sequence and of the age of the embedded cluster. The sources are probably substellar in mass, i.e., they may be young brown dwarfs.

Original languageEnglish (US)
JournalAstrophysical Journal
Volume362
Issue number1 PART 2
StatePublished - Oct 10 1990

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Ophiuchi clouds
stars

Keywords

  • Stars: brown dwarfs
  • Stars: low-mass

ASJC Scopus subject areas

  • Space and Planetary Science

Cite this

Possible substellar objects in the RHO Ophiuchi cloud. / Rieke, George H.; Rieke, Marcia J.

In: Astrophysical Journal, Vol. 362, No. 1 PART 2, 10.10.1990.

Research output: Contribution to journalArticle

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