Heavy Element Nucleosynthesis in Low Metallicity, Low Mass AGB Stars

Details Heavy Element Nucleosynthesis in Low Metallicity, Low Mass AGB Stars Heavy Element Nucleosynthesis in Low Metallicity, Low Mass AGB Stars

Mar 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003lpi....34.2043d&link_type=abstract

34th Annual Lunar and Planetary Science Conference, March 17-21, 2003, League City, Texas, abstract no.2043

Computer Science

Scientific paper

Nucleosynthesis calculations are used to predict the isotopic
compositions of Sr, Zr, Mo, Ba and Ca in low metallicity asymptotic
giant branch stars, which are believed to the source of Types Y and Z
presolar SiC grains.

Affiliated with

Also associated with

No associations

Rating

Heavy Element Nucleosynthesis in Low Metallicity, Low Mass AGB Stars 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 Heavy Element Nucleosynthesis in Low Metallicity, Low Mass AGB Stars, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Heavy Element Nucleosynthesis in Low Metallicity, Low Mass AGB Stars will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1858151