Published February 1999
| Version v1
Journal article
Colors of RR Lyrae Stars
Creators
- 1. Group P-23, University of California, Los Alamos National Laboratory (United States)
Description
The methods of Davis ampersand Cox are applied to a series of models described by Bono ampersand Stellingwerf to determine the colors of RR Lyrae stars. Convection is ignored, and the radiation flow is treated by a complete variable Eddington, multifrequency-dependent radiative transfer approximation. copyright copyright 1999. Astronomical Society of the Pacific
Additional details
Publishing Information
- Journal Title
- Publications of the Astronomical Society of the Pacific
- Journal Volume
- 111
- Journal Issue
- 756
- Journal Page Range
- p. 196-202
- ISSN
- 0004-6280
- CODEN
- PASPAU
INIS
- Country of Publication
- United States
- Country of Input or Organization
- United States
- INIS RN
- 30037897
- Subject category
- S71: CLASSICAL AND QUANTUM MECHANICS, GENERAL PHYSICS;
- Descriptors DEI
- COLOR; HERTZSPRUNG-RUSSELL DIAGRAM; HYDRODYNAMICS; MATHEMATICAL MODELS; TEMPERATURE DEPENDENCE; VARIABLE STARS
- Descriptors DEC
- DIAGRAMS; FLUID MECHANICS; INFORMATION; MECHANICS; OPTICAL PROPERTIES; ORGANOLEPTIC PROPERTIES; PHYSICAL PROPERTIES; STARS
- Proposed descriptors and Free-text terms
- RR LYRAE VARIABLE