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[*] Mass and Age of the Nuclear Star Cluster in IC 342
van der Marel R.P., Boeker T., Vacca W.
in `Dynamics of Galaxies: from the Early Universe to the Present', Combes F., Mamon G. A., Charmandaris V., eds., ASP Conference Series, Vol. 197, 271-272, 2000
© 2000. Astronomical Society of the Pacific. All Rights Reserved.

Nuclear stellar clusters are common in intermediate to late-type spirals. Here we summarize the results of a study of the mass and age of the nuclear cluster in the nearby Scd spiral IC 342, based on CO bandhead spectroscopy.

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Last modified September 20, 1999.
Roeland van der Marel, marel@stsci.edu.
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