10M Population III single and binary evolution models

T. M. Lawlor, J. MacDonald, T. R. Young

Research output: Chapter in Book/Report/Conference proceedingConference contribution

Abstract

We present stellar evolution calculations for both single and binary Population III stars, and model the effects of mass transfer. We use the structure from late stage evolution models to calculate simulated supernova lightcurves in a separate work in these proceedings.

Original languageEnglish (US)
Title of host publicationFirst Stars III
Pages238-240
Number of pages3
DOIs
Publication statusPublished - Apr 28 2008
EventFirst Stars III - Santa Fe, NM, United States
Duration: Jul 15 2007Jul 20 2007

Publication series

NameAIP Conference Proceedings
Volume990
ISSN (Print)0094-243X
ISSN (Electronic)1551-7616

Other

OtherFirst Stars III
CountryUnited States
CitySanta Fe, NM
Period7/15/077/20/07

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All Science Journal Classification (ASJC) codes

  • Physics and Astronomy(all)

Cite this

Lawlor, T. M., MacDonald, J., & Young, T. R. (2008). 10M Population III single and binary evolution models. In First Stars III (pp. 238-240). (AIP Conference Proceedings; Vol. 990). https://doi.org/10.1063/1.2905551