A copy of this work was available on the public web and has been preserved in the Wayback Machine. The capture dates from 2018; you can also visit the original URL.
The file type is
Pulsation occurs in late-type giant and supergiant stars under a wide range of atmospheric conditions and evolutionary stages. Long observational baselines are necessary to distinguish pulsation behaviors. Spectrographic and photometric observations of a variety of late-type pulsators are considered in the context of light-curve taxonomy and changing atmospheric conditions.doi:10.1515/astro-1997-0122 fatcat:j5rftakhuzdobonezjlezpe2pu