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1997A&A...328...43F - Astronomy and Astrophysics, volume 328, 43-47 (1997/12-1)
NGC 488: has its massive bulge been built up by minor mergers?
FUCHS B.
Abstract (from CDS):
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.
Abstract Copyright: ∼
Journal keyword(s): galaxies: individual: NGC 488 - galaxies: interactions - galaxies: kinematics and dynamics
Simbad objects: 1
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