New Insight into the Spatial Distribution of Novae in M31
arXiv:astro-ph/9704073 · doi:10.1086/310862
Abstract
We use a Monte Carlo technique together with a simple model for the distribution of dust in M31 to investigate the observability and spatial distribution of classical novae in M31.
18 pages, AAStex, including 6 pages of figures. Submitted ApJ Letters (March 28)
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