A Multi-resolution Statistical Method to Describe Stellar Clustering in Star-forming Dwarf Galaxies

Details A Multi-resolution Statistical Method to Describe Stellar Clustering in Star-forming Dwarf Galaxies A Multi-resolution Statistical Method to Describe Stellar Clustering in Star-forming Dwarf Galaxies

Dec 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004aas...205.9309c&link_type=abstract

American Astronomical Society Meeting 205, #93.09; Bulletin of the American Astronomical Society, Vol. 36, p.1493

Astronomy and Astrophysics

Astronomy

Scientific paper

We present a method for analyzing the large-scale distribution of resolved stars within dwarf galaxies. In particular, we are interested in determining differences in the star formation mechanisms among various types of actively star-forming dwarfs. Our primary result is the development of a well-calibrated statistical method for identifying clustering patterns.

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