Journal article
On the Origin of Sub-subgiant Stars. III. Formation Frequencies
Abstract
Sub-subgiants (SSGs) are a new class of stars that are optically redder than normal main-sequence stars and fainter than normal subgiant stars. SSGs, as well as the possibly related red stragglers (which fall to the red of the giant branch), occupy a region of the color–magnitude diagram that is predicted to be devoid of stars by standard stellar evolution theory. In previous papers we presented the observed demographics of these sources and …
Authors
Geller AM; Leiner EM; Chatterjee S; Leigh NWC; Mathieu RD; Sills A
Journal
The Astrophysical Journal, Vol. 842, No. 1,
Publisher
American Astronomical Society
Publication Date
June 10, 2017
DOI
10.3847/1538-4357/aa72ef
ISSN
0004-637X