Molecular astronomy of cool stars and sub-stellar objects

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Research output: Contribution to journal › Literature review › peer-review

Published copy (DOI)

10.1080/01442350903292442

Author(s)

Peter F. Bernath

Department/unit(s)

Chemistry

Publication details

Journal	INTERNATIONAL REVIEWS IN PHYSICAL CHEMISTRY
Date	Published - Oct 2009
Issue number	4
Volume	28
Number of pages	29
Pages (from-to)	681-709
Original language	English

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.

Research areas

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

Projects

High Resolution Infrared Laser Spectroscopy
Project: Research project (funded) › Research

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