SavedAdd your journal

Journals / Communications Faculty of Sciences University of Ankara Series A1 Mathematics and Statistics / 1961 / Cilt: 11 #74431

The density gradient in the atmosphere of the K-type component of 31 Cygni

Dilhan EZER

Pages
40–60
DOI
—

Abstract

The discovery of turbulent motions in the atmosphere of supergiant stars, made it increasingly important to study the structure of such atmospheres. The best clues to the structure of supergiant atmospheres come from the studies of eclipsing Systems.

The density gradient in the atmosphere of the K-type component of 31 Cygni — AJIndex