Published January 1984
| Version v1
Journal article
Evolutionary modelling of mass-to-luminosity ratio for galaxies of different types
Creators
- 1. Moskovskij Gosudarstvennyj Univ. (USSR). Gosudarstvennyj Astronomicheskij Inst. ''GAISh''
Description
Theoretical dependence of mass-to-luminosity ratio on the initial mass function is obtained for stellar population of galaxies of different morphological types by evolutionary population synthesis. The evolution of the mass-to-luminosity ratio is calculated for elliptical galaxies. Theoretical dependence of mass-to-luminosity ratio on the B-V colour for spiral galaxies is compared with empirical data and with other authors' models
Additional details
Additional titles
- Original title (Russian)
- Эволюционное моделирование отношения массы к светимости для галакти различных типов
Publishing Information
- Journal Title
- Astron. Zh.
- Journal Volume
- 61
- Journal Issue
- 1
- Series
- Astron. Zh.
- Journal Page Range
- 45-50
- ISSN
- 0004-6299
INIS
- Country of Publication
- Russian Federation
- Country of Input or Organization
- USSR
- INIS RN
- 16004398
- Subject category
- S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Descriptors DEI
- ELLIPTICAL CONFIGURATION; GALAXIES; LUMINOSITY; MASS; SIMULATION; SPIRAL CONFIGURATION
- Descriptors DEC
- CONFIGURATION; OPTICAL PROPERTIES; PHYSICAL PROPERTIES
Optional Information
- Notes
- For English translation see the journal Soviet Astronomy (USA).