Astronomy and Astrophysics – Astronomy
Scientific paper
Feb 1985
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985mnras.212..497b&link_type=abstract
Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 212, Feb. 1, 1985, p. 497-515. Research supported by th
Astronomy and Astrophysics
Astronomy
47
Giant Stars, Iron, Line Spectra, Metallicity, Stellar Gravitation, Equilibrium, Hydrides, Ionization, Magnesium Compounds, Pressure Broadening, Surface Properties
Scientific paper
The surface gravity of Arcturus is estimated from the strengths of MgH features (the magnesium abundance being derived from Mg I lines), from strong metal lines, and from the Fe I - Fe II ionization equilibrium. The MgH lines are log g = 1.8 (cgs units), for the effective temperature of 4375 K found by Frisk et al. (1982). This value of log g is consistent with the gravity derived from a sample of strong pressure-broadened lines of Fe I, Ca I and Na I which give log g = 1.6, and what is obtained from the ionization equilibrium of Fe, log g = 1.5. Reasons for the differences are discussed. The mass of Arcturus is found to be 0.95 solar mass when the gravity determination from MgH is used. The effective temperature is uncertain by about 50 K; a reduction of the temperature by this amount reduces the logarithmic gravity found from MgH to 1.6 and the mass to 0.7 solar mass. It is concluded that the MgH features offer promising possibilities for determining gravities of late-type stars, when good estimates of effective temperatures are available.
Bell Roger A.
Edvardsson Bengt
Gustafsson Bengt
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