Molecular astronomy of cool stars and sub-stellar objects

Research output: Contribution to journalLiterature reviewpeer-review

Abstract

The optical and infrared spectra of a wide variety of 'cool' astronomical objects including the Sun, sunspots, K-, M- and S-type stars, carbon stars, brown dwarfs and extrasolar planets are reviewed. The review provides the necessary astronomical background for chemical physicists to understand and appreciate the unique molecular environments found in astronomy. The calculation of molecular opacities needed to simulate the observed spectral energy distributions is discussed.

Original languageEnglish
Pages (from-to)681-709
Number of pages29
JournalINTERNATIONAL REVIEWS IN PHYSICAL CHEMISTRY
Volume28
Issue number4
DOIs
Publication statusPublished - Oct 2009

Keywords

  • extrasolar planets
  • cool stars
  • brown dwarfs
  • solar spectra
  • sunspots
  • spectral energy distributions
  • molecular opacities
  • astronomical spectroscopy
  • INFRARED-EMISSION SPECTROSCOPY
  • RESOLUTION SPECTRAL ATLAS
  • GIANT BRANCH STARS
  • ALL-SKY SURVEY
  • LOW-MASS STARS
  • CARBON STARS
  • MU-M
  • S-STARS
  • SOLAR GRANULATION
  • LINE FORMATION

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