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Short-duration radio flares of UV Ceti starsThe UV Ceti-type stars YZ Canis Minoris, AD Leonis, Wolf 424, and V371 Orionis were monitored with the Arecibo radio telescope at meter wavelengths. A total of 26 flares were recorded on YZ CMi, AD Leo, and Wolf 424. The observed flares had shorter durations and smaller amplitudes than those previously reported in the literature. Rates of radio-flare detection are similar to those found optically.
Document ID
19740052291
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
External Source(s)
Authors
Spangler, S. R.
Shawhan, S. D.
Rankin, J. M.
(Iowa, University Iowa City, Iowa, United States)
Date Acquired
August 7, 2013
Publication Date
June 15, 1974
Publication Information
Publication: Astrophysical Journal
Volume: 190
Subject Category
Space Sciences
Accession Number
74A35041
Funding Number(s)
CONTRACT_GRANT: NGL-16-001-002
CONTRACT_GRANT: NSF GA-37827
Distribution Limits
Public
Copyright
Other

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