Stellar Physics Using High-Resolution Spectroscopy with Large Telescopes

Details Stellar Physics Using High-Resolution Spectroscopy with Large Telescopes Stellar Physics Using High-Resolution Spectroscopy with Large Telescopes

Oct 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995pasp..107..994d&link_type=abstract

Publications of the Astronomical Society of the Pacific, v.107, p.994

Astronomy and Astrophysics

Astronomy

1

Instrumentation: Spectrographs, Techniques: Spectroscopy

Scientific paper

The traditional high resolution domain of stellar physics will be profoundly affected by the deployment of 8-10 meter class telescopes. We discuss here some of the advances anticipated in the fields of stellar convection, seismology and magentic structures. Also discussed are the tests of stellar evolution and star formation processes that one may expect based on high resolution observations of radial velocity, Doppler imaging, and chemical abundances. (SECTION: Workshop on High-Resolution Spectroscopy)

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