Computer Science
Scientific paper
Mar 2008
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008aipc..990..325c&link_type=abstract
FIRST STARS III: First Stars II Conference. AIP Conference Proceedings, Volume 990, pp. 325-329 (2008).
Computer Science
1
Supergiant Stars, Abundances, Chemical Composition, Stellar Rotation, Population Iii Stars, Stellar Structure, Interiors, Evolution, Nucleosynthesis, Ages
Scientific paper
Rapidly rotating massive stars are currently one of the most promising ways of explaining the high N/O abundances measured in normal metal poor stars. Here we show the predicted impact of fast rotators on the 12C/13C ratio at very low metallicities. We show that upon the inclusion of fast rotating massive stars, low 12C/13C ratios are expected in extremely metal poor halo stars. Observations of 12C/13C ratios in metal poor dwarf and turnoff stars would offer a crucial test to the idea that fast rotating stars were a common phenomenona in the primordial Universe.
Chiappini Cristina
Ekstrom Sylvia
Hirschi Raphael
Maeder Andre
Meynet Georges
No associations
LandOfFree
Were the First Stars Fast Rotators? 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 Were the First Stars Fast Rotators?, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Were the First Stars Fast Rotators? will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1036942