University of Hertfordshire

By the same authors

Water and titanium oxide in late-type M dwarfs

Research output: Chapter in Book/Report/Conference proceedingConference contribution

Documents

  • H.R.A. Jones
  • S. Viti
  • S. Miller
  • J. Tennyson
  • F. Allard
  • P. Hauschildt
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Original languageEnglish
Title of host publicationIn: Cool stars, stellar systems and the sun 9, ASP Conference Series 109
PublisherAstronomical Society of the Pacific
Pages717-8
ISBN (Print)1-886733-29-5
Publication statusPublished - 1996

Abstract

Despite the identification of brown dwarf candidates the lack of understanding of M dwarfs has meant that it has not been possible to unambiguously distinguish these candidates from cool M dwarfs. Unlike hotter stars their atmospheres are dominated by a variety of species of molecules, many with billions of line transitions modulating their energy output. We have recently examined water vapour and titanium oxide opacities which are the most important sources of opacity in cool low-mass stars.

Notes

Original paper can be found at: http://www.astrosociety.org/pubs/cs/070-112.html--Copyright Astronomical Society of the Pacific

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