The influence of CN abundances on the evolution of main sequence of low-mass stars

Details The influence of CN abundances on the evolution of main sequence of low-mass stars The influence of CN abundances on the evolution of main sequence of low-mass stars

Jul 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982a%26a...111..312b&link_type=abstract

Astronomy and Astrophysics, vol. 111, no. 2, July 1982, p. 312-316.

Astronomy and Astrophysics

Astrophysics

13

Abundance, Cyanogen, Main Sequence Stars, Stellar Evolution, Cyano Compounds, Globular Clusters, Stellar Luminosity, Stellar Mass

Scientific paper

Theoretical isochrones are derived for mild metal-poor (Fe/H abundance ratios of approximately -0.7) stars under various assumptions on the relative amount of CNO elements. Cluster ages in the range 8-18 billion yr are explored, showing that the turn-off luminosity decreases with increasing CNO content according to a certain relation. The consequences of these determinations of cluster age are discussed.

Affiliated with

Also associated with

No associations

Rating

The influence of CN abundances on the evolution of main sequence of low-mass 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 The influence of CN abundances on the evolution of main sequence of low-mass stars, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The influence of CN abundances on the evolution of main sequence of low-mass stars will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1022102