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Isolated cores in early-type disk galaxies: NGC 4672

Abstract:

The morphological features of the early-type disk galaxy NGC 4672 are discussed as well as the velocity curves and velocity dispersion profiles of stars and ionized gas along both its major and minor axes. We conclude that NGC 4672 has structural (i.e. a bulge elongated perpendicularly to the disk) and kinematical (i.e, a stellar core rotating perpendicularly to the disk) properties similar to those of the Sa NGC 4698. The presence of the isolated core suggests that the disk component is the ...

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Publication status:
Published

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Institution:
University of Oxford
Division:
MPLS
Department:
Physics
Sub department:
Astrophysics
Role:
Author
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Journal:
STARS, GAS AND DUST IN GALAXIES: EXPLORING THE LINKS, PROCEEDINGS
Volume:
221
Pages:
249-252
Publication date:
2000-01-01
Event title:
CTIO/ESO/LCO Joint Workshop on Stars, Gas and Dust in Galaxies
Source identifiers:
15353
ISBN:
1583810536
Keywords:
Pubs id:
pubs:15353
UUID:
uuid:ccaa93c7-4636-4e5e-9eff-4fdeb13ae68e
Local pid:
pubs:15353
Deposit date:
2012-12-19

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