NGC 488: Has its massive bulge been build up by minor mergers?

Details NGC 488: Has its massive bulge been build up by minor mergers? NGC 488: Has its massive bulge been build up by minor mergers?

1997-08-04

arxiv.org/abs/astro-ph/9708029v1

Astronomy and Astrophysics

Astrophysics

Latex, 6 pages, 5 figures, to appear in A&A

Scientific paper

Using recent observations of the kinematics of the disk stars the dynamical
state of the disk of NGC 488 is discussed. The disk is shown to be dynamically
`cool', so that NGC 488 cannot have experienced many -- even minor -- mergers
in the past.

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