Evidence for a triaxial bulge in the spiral galaxy NGC 4845
Journal Article
·
· Astrophysical Journal; (USA)
- Padova Universita, Padua (Italy) Carnegie Institution of Washington, Washington, DC (USA)
Spectroscopic observations for the Sa galaxy NGC 4845 in five position angles reveal a regular but nonaxisymmetric velocity field for the gas at r of 1.5 kpc or less. Photometry indicates a possible slight twisting between the disk and bulge isophotes. These phenomena are interpreted as a manifestation of a triaxial bulge, and estimates of the ranges of b/a and c/a are obtained. 20 refs.
- OSTI ID:
- 5095698
- Journal Information:
- Astrophysical Journal; (USA), Vol. 345; ISSN 0004-637X
- Country of Publication:
- United States
- Language:
- English
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The triaxial bulge of the Sa galaxy NGC 4845
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OSTI ID:5095698
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Tue Jan 20 00:00:00 EST 2015
· Astrophysical Journal
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OSTI ID:5095698