Long-term variability and possible stellar cycles in hybrid-chromosphere starsResults from an investigation of the variability seen in the Mg II emission line fluxes and wind absorption components of a number of hybrid-chromosphere stars are presented. One star shows evidence of stellar cycle activity with a period on the order of 2000 days.
Document ID
19910060275
Acquisition Source
Legacy CDMS
Document Type
Conference Paper
Authors
Veale, Anthony W. (Joint Inst. for Lab. Astrophysics Boulder, CO, United States)
Brown, Alexander (Joint Institute for Laboratory Astrophysics Boulder, CO, United States)