Outer atmospheres of cool stars observed with IUE

Details Outer atmospheres of cool stars observed with IUE Outer atmospheres of cool stars observed with IUE

Dec 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984nascp2349...64b&link_type=abstract

In NASA. Goddard Space Flight Center Future of Ultraviolet Astronomy Based on Six Years of IUE Res. p 64-79 (SEE N85-20961 11-8

Astronomy and Astrophysics

Astronomy

2

Atmospheric Heating, Iue, Stellar Atmospheres, Stellar Flares, Ultraviolet Astronomy, Emission Spectra, Magnetic Fields, Stellar Evolution, Stellar Winds, Time Series Analysis, X Ray Sources

Scientific paper

Ultrviolet observations of cool stars in conjuction with coronal X-ray or ground based chromospheric measurements, or both have served both to refine and define understanding of stellar activity. The sensitivity of IUE down to a reasonable limiting magnitude made accessible many different stars' ultraviolet spectra. Understanding of stellar activity throughout stellar atmospheres has progressed because observation in the ultraviolet range of particular stars can be done in great detail.

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