Abstract
Abstract
Evidence is presented that the far ultraviolet flux of Maia recorded by the International Ultraviolet Explorer is variable over a timescale of a few hours. In contrast, the radial velocity of the Si ii doublet near 1530 Å does not vary on short timescales.
Publisher
American Astronomical Society
Cited by
1 articles.
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1. Maia variables and other anomalies among pulsating stars;Frontiers in Astronomy and Space Sciences;2023-09-14