A Connection between the Morphology of the X-Ray Emission and Rotation for Solar-Type Stars in Open Clusters
Year: 2003
Type: article
Abstract: It is suggested that the three-segmented morphology of the soft X-ray emission from cluster and field stars may be understood in terms of the recent classification of rotating stars into three kinds: those lying on the convective sequence, on the interface sequence, or in the gap between them.
Source: The Astrophysical Journal
DOI: 10.1086/374681
Author: Sydney A. Barnes
Institution: Yale University
Language: English
Subfield: Astronomy and Astrophysics
Field: Physics and Astronomy
Domain: Physical Sciences
Open Access status: bronze
OpenAlex ID: W2026655774