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Super Star Clusters in NGC 7673 and Mrk 8

Published online by Cambridge University Press:  03 August 2017

N. Homeier  and
J.S. Gallagher
N. Homeier
Affiliation:
University of Wisconsin-Madison, 475 N. Charter St., Sterling Hall, Madison, WI 53706, USA
J.S. Gallagher
Affiliation:
University of Wisconsin-Madison, 475 N. Charter St., Sterling Hall, Madison, WI 53706, USA

Abstract

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We present an analysis of super star cluster populations using WFPC 2 on the Hubble Space Telescope for two starburst galaxies: NGC 7673 and Markarian 8. Both galaxies are luminious and have signatures of massive star formation, such as emission-line dominated optical spectra. Their optical appearances are highly disturbed, featuring prominent knots of intense star formation. Using HST F255W, F555W, and F814W images, we perform aperture photometry for a select sample of star clusters in different regions of each galaxy, and compare the results with evolutionary population synthesis models.

Type
Part 3. Super Star Clusters and Associations
Information
Symposium - International Astronomical Union , Volume 207: Extragalactic Star Clusters , 2002 , pp. 464 - 467
Copyright
Copyright © Astronomical Society of the Pacific 2002 

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