Ultraviolet spectroscopy of cool stars

Details Ultraviolet spectroscopy of cool stars Ultraviolet spectroscopy of cool stars

Oct 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988josab...5.2252j&link_type=abstract

Optical Society of America, Journal, B: Optical Physics (ISSN 0740-3224), vol. 5, Oct. 1988, p. 2252-2263.

Computer Science

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13

Cool Stars, Dwarf Stars, Main Sequence Stars, Stellar Spectra, Ultraviolet Astronomy, Chromosphere, Giant Stars, Rocket Sounding, Satellite Observation, Stellar Coronas

Scientific paper

A review is given of some developments in the study of UV emission-line spectra of cool stars, including the Sun, in recent years. Observations of cool low-gravity stars (giants and supergiants) with the International Ultraviolet Explorer have led to the discovery of a variety of fluorescent excitation processes, some resulting in the determination of further energy levels. Some examples of line-identification problems and excitation processes are discussed.

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