Masses and mass-to-light ratios of galaxies.
Abstract
The current status of the 'missing mass' problem is reviewed on the basis of standardized mass-to-light (M/L) ratios of galaxies. The stellar mass density in the immediate vicinity of the sun is examined, along with the mass of the Milky Way and the M/L ratios of spiral galaxies, E and S0 galaxies, and binary galaxies. The dynamics of small groups of galaxies is investigated, and mass derivations for cluster galaxies are discussed. It is concluded that the case for invisible mass in the universe is very strong and becoming stronger.
- Publication:
-
Annual Review of Astronomy and Astrophysics
- Pub Date:
- 1979
- DOI:
- 10.1146/annurev.aa.17.090179.001031
- Bibcode:
- 1979ARA&A..17..135F
- Keywords:
-
- Galactic Clusters;
- Light Curve;
- Mass To Light Ratios;
- Spiral Galaxies;
- Disk Galaxies;
- Dynamic Response;
- Galactic Structure;
- Group Theory;
- Mass Distribution;
- Milky Way Galaxy;
- Missing Mass (Astrophysics);
- Stellar Luminosity;
- Stellar Mass Ejection;
- Astrophysics;
- Galaxies:Mass-to-Light Ratios;
- Galaxies:Masses;
- Galaxies:Missing Mass;
- Galaxy:Mass;
- Groups of Galaxies:Dynamics;
- Groups of Galaxies:Mass-to-Light Ratios