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T.M. Lawlor (Penn State University Wilkes-Barre), J. MacDonald (University of Delaware), T.R. Young (University of North Dakota)
We present preliminary models that explore the effect of mass transfer on to a massive AGB star, which is expected to later undergo a supernova outburst. We include models of various masses and metallicities, including a very low Z model appropriate to the first stars formed in the early universe.
The author(s) of this abstract have provided an email address for comments about the abstract: tlawlor@psu.edu
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Bulletin of the American Astronomical Society, 37 #2
© 2005. The American Astronomical Soceity.