The Semistellar Nucleus of M33
Spectroscopic observations suggest that the light emitted by the semistellar nucleus of M33 is dominated by relatively young stars. This observation indicates that the nuclei of some galaxies may be formed from interstellar gas rather than from an accumulation of globular clusters.
- Research Organization:
- David Dunlap Observatory, University of Toronto, Richmond Hill, Ontario, Canada
- Sponsoring Organization:
- USDOE
- NSA Number:
- NSA-33-030820
- OSTI ID:
- 4026957
- Journal Information:
- Astrophysical Journal, Vol. 203; Other Information: Orig. Receipt Date: 30-JUN-76; ISSN 0004-637X
- Publisher:
- Institute of Physics (IOP)
- Country of Publication:
- United States
- Language:
- English
Similar Records
Star formation in the semistellar nucleus of M33
Structure of the M33 nucleus
The stellar populations of M 33
Journal Article
·
Fri Apr 01 00:00:00 EST 1983
· Astrophys. J.; (United States)
·
OSTI ID:4026957
Structure of the M33 nucleus
Journal Article
·
Wed Dec 01 00:00:00 EST 1982
· Astrophys. J.; (United States)
·
OSTI ID:4026957
The stellar populations of M 33
Journal Article
·
Mon Jul 01 00:00:00 EDT 1991
· Publications of the Astronomical Society of the Pacific; (United States)
·
OSTI ID:4026957