Mid-mass Population III Stars: Evolution, Structure, Composition And Mass Loss.

Details Mid-mass Population III Stars: Evolution, Structure, Composition And Mass Loss. Mid-mass Population III Stars: Evolution, Structure, Composition And Mass Loss.

Jan 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009aas...21340712l&link_type=abstract

American Astronomical Society, AAS Meeting #213, #407.12; Bulletin of the American Astronomical Society, Vol. 41, p.204

Astronomy and Astrophysics

Astronomy

Scientific paper

We present model results for mid-mass Population III stars. While Bodies of work investigating high and very high mass population III model stars are becoming abundant, as is true for low mass models, there remains a dearth of studies in the intermediate range. We include and describe the effects of an expanded reaction network, and examine what yields are produced via late stage evolution mass loss. We intend to extend our grid of models to include the effects of close binary evolution and ultimately will model the resulting supernova light curves.

Affiliated with

Also associated with

No associations

Rating

Mid-mass Population III Stars: Evolution, Structure, Composition And Mass Loss. does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Mid-mass Population III Stars: Evolution, Structure, Composition And Mass Loss., we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Mid-mass Population III Stars: Evolution, Structure, Composition And Mass Loss. will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1701524