Six new rapidly oscillating Ap stars in the Kepler long-cadence data using super-Nyquist asteroseismology (2019)
Attributed to:
Consolidated Solar and Astrophysics Research at UCLan
funded by
STFC
Abstract
No abstract provided
Bibliographic Information
Digital Object Identifier: http://dx.doi.org/10.48550/arxiv.1906.04353
Publication URI: https://arxiv.org/abs/1906.04353
Type: Other