Plane-parallel VS spherical geometry vis-a-vis scale-heights

Details Plane-parallel VS spherical geometry vis-a-vis scale-heights Plane-parallel VS spherical geometry vis-a-vis scale-heights

May 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982ap%26ss..84..155v&link_type=abstract

Astrophysics and Space Science, vol. 84, no. 1, May 1982, p. 155-161.

Astronomy and Astrophysics

Astrophysics

1

Atmospheric Models, Scale Height, Stellar Atmospheres, Depth, Interferometry, Omicron Ceti Star, Spherical Coordinates

Scientific paper

The g(min) values above which plane-parallel approximation should provide satisfactory model atmospheres are computed, in a theoretical study which makes use of the Kurucz et al. (1974) plane-parallel atmosphere tabulations. Corroborative evidence for the high g(min) values arrived at is found in the Labeyrie et al. (1977) speckle interferometry measurement of the Mira star Omicron Ceti's diameter.

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