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The Temperature of the Supergiant α Per1
Published online by Cambridge University Press: 12 April 2016
Abstract
We compare observed fluxes from the ultraviolet (IUE) through J and K with recent Kurucz model atmospheres to determine a temperature for the F5 lb supergiant α Per. The two most important advances in this study as compared with previous work are the use of well calibrated ultraviolet fluxes and the use of models with an appropriate microturbulence.
- Type
- Part 2. Poster Papers
- Information
- International Astronomical Union Colloquium , Volume 155: Astrophysical Applications of Stellar Pulsation , 1995 , pp. 393 - 394
- Copyright
- Copyright © Astronomical Society of the Pacific 1995
Footnotes
Staff Member of the International Ultraviolet Explorer Observatory
IUE Archival Research