Skip to main content
OSTI.GOVU.S. Department of Energy Office of Scientific and Technical Information
U.S. Department of Energy
Office of Scientific and Technical Information
 

Difference at chromospheric levels between rs cvn-type binaries, active and quiet chromosphere single stars, and active and quiet regions in the sun

Technical Report ·
OSTI ID:5913303

This paper summarizes the differences in the properties of active chromospheres compared with quiet chromospheres by comparing active and quiet regions on the Sun, active and quiet chromosphere stars, and the very active chromospheres seen in close binary systems with chromospheres of single stars. In particular, the chromospheres of the RS CVn-type binary systems UX Arietis and HR 1099 and the chromosphere of UX Arietis during a flare are modeled.

Research Organization:
National Bureau of Standards, Washington, DC (USA)
OSTI ID:
5913303
Report Number(s):
PB-81-149288
Country of Publication:
United States
Language:
English

Similar Records

A study of active regions on RS CVn stars
Thesis/Dissertation · Sat Dec 31 23:00:00 EST 1988 · OSTI ID:6105074
Multiple wavelength microwave observations of the RS Canum Venaticorum stars UX Arietis, HR 1099, HR 5110, and II Pegasi
Journal Article · Wed Dec 31 23:00:00 EST 1986 · Astrophys. J.; (United States) · OSTI ID:6581574
Radio observations of the binary stars UX Arietis and HR 1099
Journal Article · Mon Jan 31 23:00:00 EST 1977 · Astron. J.; (United States) · OSTI ID:7325684

Related Subjects

640102 -- Astrophysics & Cosmology-- Stars & Quasi-Stellar
Radio & X-Ray Sources
640104* -- Astrophysics & Cosmology-- Solar Phenomena
71 CLASSICAL AND QUANTUM MECHANICS
GENERAL PHYSICS
ATMOSPHERES
BINARY STARS
CHROMOSPHERE
MAIN SEQUENCE STARS
SOLAR ATMOSPHERE
SPECTRA
STARS
STELLAR ATMOSPHERES
STELLAR FLARES
SUN
ULTRAVIOLET SPECTRA