The ZAHB luminosity-metallicity relationship as derived from main sequence fitting

Details The ZAHB luminosity-metallicity relationship as derived from main sequence fitting The ZAHB luminosity-metallicity relationship as derived from main sequence fitting

Apr 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990a%26a...230..315b&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 230, no. 2, April 1990, p. 315-325. Research supported by CNR and MPI.

Astronomy and Astrophysics

Astrophysics

24

Globular Clusters, Horizontal Branch Stars, Main Sequence Stars, Metallicity, Stellar Luminosity, Abundance, Galactic Clusters, Metallic Stars, Stellar Evolution

Scientific paper

A detailed revision of a study of the luminosity-metallicity relationship of the zero age horizontal branch (ZAHB) stars in Galactic globular clusters is presented in order to clear up conflicting results obtained by Buonanno et al. (1989) and King et al. (1988). The results show that the discrepancy is due mostly to differences in their adopted procedures.

Affiliated with

Also associated with

No associations

Rating

The ZAHB luminosity-metallicity relationship as derived from main sequence fitting 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 ZAHB luminosity-metallicity relationship as derived from main sequence fitting, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The ZAHB luminosity-metallicity relationship as derived from main sequence fitting will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1379300