STELLAR PHYSICS USING HIGH-RESOLUTION SPECTROSCOPY WITH LARGE TELESCOPES

Authors
Citation
P. Demarque, STELLAR PHYSICS USING HIGH-RESOLUTION SPECTROSCOPY WITH LARGE TELESCOPES, Publications of the Astronomical Society of the Pacific, 107(716), 1995, pp. 994-996
Citations number
1
Categorie Soggetti
Astronomy & Astrophysics
Journal title
Publications of the Astronomical Society of the Pacific
ISSN journal
00046280 → ACNP
Volume
107
Issue
716
Year of publication
1995
Pages
994 - 996
Database
ISI
SICI code
0004-6280(1995)107:716<994:SPUHSW>2.0.ZU;2-Y
Abstract
The traditional high-resolution domain of stellar physics will be affe cted profoundly by the deployment of 8-10-m class telescopes. We discu ss here some of the advances anticipated in the fields of stellar conv ection, seismology, and magnetic structures. Also discussed are the te sts of stellar evolution and star-formation processes than one may exp ect based on high-resolution observations of radial velocity, Doppler imaging, and chemical abundances.