Determination of C, N, O abundances in the atmosphere of beta Lyrae from infrared spectra

Details Determination of C, N, O abundances in the atmosphere of beta Lyrae from infrared spectra Determination of C, N, O abundances in the atmosphere of beta Lyrae from infrared spectra

Apr 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980sval....6...94l&link_type=abstract

(Pis'ma v Astronomicheskii Zhurnal, vol. 6, Mar. 1980, p. 171-174.) Soviet Astronomy Letters, vol. 6, Mar.-Apr. 1980, p. 94-96.

Astronomy and Astrophysics

Astronomy

2

Abundance, Binary Stars, Carbon Stars, Infrared Astronomy, Chemical Composition, Stellar Atmospheres

Scientific paper

Abundances of the elements participating in the C, N, O cycle are
derived from near-infrared spectra of beta Lyr. The material in the
atmosphere of the bright component has undergone hydrogen burning via
this cycle. Estimates are obtained for the present as well as the
initial mass of the bright component in this binary system.

Affiliated with

Also associated with

No associations

Rating

Determination of C, N, O abundances in the atmosphere of beta Lyrae from infrared spectra 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 Determination of C, N, O abundances in the atmosphere of beta Lyrae from infrared spectra, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Determination of C, N, O abundances in the atmosphere of beta Lyrae from infrared spectra will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1700048