Astronomy and Astrophysics – Astrophysics
Scientific paper
Apr 1986
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986a%26as...64..173a&link_type=abstract
Astronomy and Astrophysics Supplement Series (ISSN 0365-0138), vol. 64, no. 1, April 1986, p. 173-187. Research supported by the
Astronomy and Astrophysics
Astrophysics
26
A Stars, Abundance, B Stars, Stellar Composition, Atmospheric Models, Line Spectra, Stellar Spectrophotometry, Tables (Data), Ubv Spectra
Scientific paper
Abundance analyses using optical region data and fully line-blanketed model atmospheres have been performed for four sharp-lined normal B and A type stars. This work extends the results presented in the first and fourth papers of this series. The microturbulent velocities of all the stars studied in this series are found to follow the same relation with temperature. Some of the stars studied in this paper are found to have one or two anomalous abundances, such as the zirconium abundance of θ Leo.
No associations
LandOfFree
Optical region elemental abundance analyses of B and A stars. V - The normal stars Theta Leonis, Tau Herculis, 14 Cygni, and 5 Aquarii 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 Optical region elemental abundance analyses of B and A stars. V - The normal stars Theta Leonis, Tau Herculis, 14 Cygni, and 5 Aquarii, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Optical region elemental abundance analyses of B and A stars. V - The normal stars Theta Leonis, Tau Herculis, 14 Cygni, and 5 Aquarii will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1101408