Astronomy and Astrophysics – Astrophysics
Scientific paper
Mar 1979
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979s%26w....18...82b&link_type=abstract
Sterne und Weltraum, vol. 18, Mar. 1979, p. 82-87. In German.
Astronomy and Astrophysics
Astrophysics
Nuclear Reactions, Red Giant Stars, Stellar Evolution, Stellar Spectra, Abundance, Anomalies, Cool Stars, Hertzsprung-Russell Diagram, Nuclear Astrophysics, Spectral Bands, Stellar Atmospheres
Scientific paper
Analysis of various anomalous spectra of developed cool stars shows that these spectra can largely be accounted for by anomalous chemical compositions of the atmospheres of the stars. The means of transport of burning products to the outer layers is still undetermined. Abundance anomalies in S-stars and cool C-stars can be attributed to the operating of neutron processes corresponding to the Ne-22 mechanism.
No associations
LandOfFree
Anomalous spectra of red giants - Nuclear reactions and mixing processes during star development 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 Anomalous spectra of red giants - Nuclear reactions and mixing processes during star development, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Anomalous spectra of red giants - Nuclear reactions and mixing processes during star development will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-809518