The Neon Abundance in WR Stars: Testing Massive Star Evolution

Details The Neon Abundance in WR Stars: Testing Massive Star Evolution The Neon Abundance in WR Stars: Testing Massive Star Evolution

Jun 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008aspc..388..233w&link_type=abstract

Mass Loss from Stars and the Evolution of Stellar Clusters ASP Conference Series, Vol. 388, proceedings of the conference held 2

Astronomy and Astrophysics

Astronomy

Scientific paper

The neon abundance in WR stars provides one of the most sensitive tests
of massive star evolution theory being predicted to undergo enhancements
of ×10 (WC phase) up to ×100 (WO phase). Results from ISO
are summarized and our new IR programme with the Spitzer satellite is
outlined.

Affiliated with

Also associated with

No associations

Rating

The Neon Abundance in WR Stars: Testing Massive Star Evolution 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 The Neon Abundance in WR Stars: Testing Massive Star Evolution, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The Neon Abundance in WR Stars: Testing Massive Star Evolution will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-989330