Age and Initial Helium Abundance of Globular Cluster Stars

Details Age and Initial Helium Abundance of Globular Cluster Stars Age and Initial Helium Abundance of Globular Cluster Stars

Aug 1969

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1969natur.223..933i&link_type=abstract

Nature, Volume 223, Issue 5209, pp. 933-934 (1969).

Other

35

Scientific paper

IT has already been shown that the number of horizontal branch stars (NHB) relative to the number of red giant stars (NRG) brighter than an appropriate magnitude could be used together with other observable cluster characteristics to estimate the age and initial helium abundance of stars in globular clusters1.

Affiliated with

Also associated with

No associations

Rating

Age and Initial Helium Abundance of Globular Cluster 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 Age and Initial Helium Abundance of Globular Cluster Stars, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Age and Initial Helium Abundance of Globular Cluster Stars will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1690358