Physical conditions in the atmospheres of M giants

Details Physical conditions in the atmospheres of M giants Physical conditions in the atmospheres of M giants

Feb 1977

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1977sva....21...26k&link_type=abstract

(Astronomicheskii Zhurnal, vol. 54, no. 1, 1977, p. 48-54.) Soviet Astronomy, vol. 21, Jan.-Feb. 1977, p. 26-29. Translation.

Astronomy and Astrophysics

Astronomy

1

Giant Stars, M Stars, Spectrum Analysis, Stellar Atmospheres, Stellar Evolution, Stellar Models, Atmospheric Composition, Classifications, Stellar Spectra, Stellar Temperature

Scientific paper

Results are reported for analysis of 15 spectrograms of the M giants Delta-2 Lyr and g Her, which were obtained with a reciprocal dispersion of 14 A/mm over the wavelength range from 3900 to 4700 A. Physical parameters of the stellar atmospheres at each moment of observation are determined by the curve-of-growth technique, and vibrational-excitation temperatures are estimated from alpha-system bands of TiO. For Delta-2 Lyr, a logarithmic electron pressure of -5.87 and a logarithmic gas pressure of -1.5 are computed; for g Her, the respective values are -4.85 and -0.5.

Affiliated with

Also associated with

No associations

Rating

Physical conditions in the atmospheres of M giants 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 Physical conditions in the atmospheres of M giants, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Physical conditions in the atmospheres of M giants will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-800872