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