A new method for the asteroseismic determination of the evolutionary state of red-giant stars (2017)
Attributed to:
Asteroseismology and Helioseismology at Birmingham and Queen Mary
funded by
STFC
Abstract
No abstract provided
Bibliographic Information
Digital Object Identifier: http://dx.doi.org/10.1093/mnras/stw3288
Publication URI: http://dx.doi.org/10.1093/mnras/stw3288
Type: Journal Article/Review
Parent Publication: Monthly Notices of the Royal Astronomical Society
Issue: 3