Dynamical implications of multiple stellar populations

Details Dynamical implications of multiple stellar populations Dynamical implications of multiple stellar populations

Aug 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007hia....14..436s&link_type=abstract

Highlights of Astronomy, Volume 14, p. 436-437

Astronomy and Astrophysics

Astronomy

Stars: Agb And Post-Agb, Globular Clusters: General, Globular Clusters: Individual (Ngc 2808)

Scientific paper

We investigate some implications of having two star formation episodes in globular clusters, rather than the traditional single-burst approximation. Evidence for more than one stellar generation is accumulating in observations of abundances of elements lighter than iron in globular cluster stars, and is thought to imply some self-enrichment of the globular cluster gas. In particular, we explore models based on the assumption that the self-enrichment comes from an early generation of asymptotic giant branch (AGB) stars.

Affiliated with

Also associated with

No associations

Rating

Dynamical implications of multiple stellar populations 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 Dynamical implications of multiple stellar populations, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Dynamical implications of multiple stellar populations will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-974834