Published March 1985
| Version v1
Journal article
Spectral classes of the cold components of U Gem type stars
Description
A relationship has been found between the orbital period of U Gem binary systems and the spectral class of their cold components. The existence of this relation may make it possible to determine the spectral class of the cold components of such stars that are difficult to observe. In addition, it follows from the orbital-period-mass and orbital-periodspectral-class relations of the cold components that they are on the main sequence. This makes it possible to estimate the luminosities of the cold components from the revolution period
Additional details
Publishing Information
- Journal Title
- Astrophysics (Engl. Transl.)
- Journal Volume
- 20
- Journal Issue
- 5
- Series
- Astrophysics (Engl. Transl.).
- Journal Page Range
- 507-510
- ISSN
- 0004-6396
- CODEN
- ATPYA
INIS
- Country of Publication
- United States
- Country of Input or Organization
- United States
- INIS RN
- 18003779
- Subject category
- S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Descriptors DEI
- ALGORITHMS; BINARY STARS; CORRELATIONS; EMISSION SPECTRA; LUMINOSITY; ORBITS
- Descriptors DEC
- OPTICAL PROPERTIES; PHYSICAL PROPERTIES; SPECTRA; STARS
Optional Information
- Notes
- Translated from Astrofizika, Vol. 21, No. 5, pp. 289-294, September-October, 1984.. Cover-to-cover translation of Astrofizika (USSR).