Published February 1986 | Version v1
Journal article Metadata-only

Choice of a model for Z Andromedae

Creators

  • 1. Moskovskii Gosudarstvennyi Universitet, Moscow, USSR

Description

Data from recent visible-range spectrophotometric observations of Z And (Blair et al., 1983; Ipatov and Iudin, 1985) are combined with data from previous observations and analyzed. Alternative models of the cool component, nebula, and hot component are characterized in detail, and it is concluded that no choice is yet possible between models with accreting-white-dwarf and red-dwarf hot components. 35 references

Additional details

Publishing Information

Journal Title
Sov. Astron. (Engl. Transl.)
Journal Volume
30
Series
Sov. Astron. (Engl. Transl.).
Journal Page Range
84-92
ISSN
0038-5301
CODEN
SAAJA

INIS

Country of Publication
United States
Country of Input or Organization
United States
INIS RN
18063348
Subject category
S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
Descriptors DEI
ACCRETION DISKS; BINARY STARS; LUMINOSITY; MAIN SEQUENCE STARS; RED DWARF STARS; SPECTROPHOTOMETRY; STAR ACCRETION; STAR MODELS; SYMBIOTIC STARS; WHITE DWARF STARS
Descriptors DEC
DWARF STARS; MATHEMATICAL MODELS; OPTICAL PROPERTIES; PHYSICAL PROPERTIES; STAR EVOLUTION; STARS

Optional Information

Notes
Cover-to-cover translation of Astronomicheskij Zhurnal (USSR).