Astronomy and Astrophysics – Astronomy
Scientific paper
Apr 1984
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984azh....61..333g&link_type=abstract
(Astronomicheskii Zhurnal, vol. 61, Mar.-Apr. 1984, p. 333-342) Soviet Astronomy (ISSN 0038-5301), vol. 28, Mar.-Apr. 1984, p. 1
Astronomy and Astrophysics
Astronomy
8
A Stars, G Stars, Spectral Energy Distribution, Stellar Atmospheres, Stellar Models, Stellar Spectra, Stellar Spectrophotometry, Stellar Temperature, Emission Spectra, Radii, Stellar Gravitation, Stellar Luminosity
Scientific paper
The effective temperatures, bolometric corrections, radii, and values of the acceleration of gravity are determined for 20 A-G stars of different luminosity classes on the basis of extra-atmospheric and ground-based data on the spectral energy distribution. A comparison with Kurucz's (1979) theoretical models shows that for stars earlier than A7, the theoretical models in the range of 3200-10,800 A agree well with observations, while for the later stars the observed energy distribution in the ultraviolet region lies below the theoretical distribution down to Te = 5500 K, the minimum temperature in Kurucz's models.
No associations
LandOfFree
Effective temperatures of stars of spectral classes A-G Comparison with theoretical models 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 Effective temperatures of stars of spectral classes A-G Comparison with theoretical models, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Effective temperatures of stars of spectral classes A-G Comparison with theoretical models will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1499141