Previous | Session 93 | Next
C. Czech, M. M. Crone (Skidmore College)
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.
Previous | Session 93 | Next
Bulletin of the American Astronomical Society, 36 5
© 2004. The American Astronomical Society.