Journal article
A search for slowly varying radio continuum emission from UV Ceti stars
The Astrophysical journal, Vol.205, p.472
04/1976
DOI: 10.1086/154300
Abstract
The paper presents results of a search conducted at the Arecibo Observatory for variable 430-MHz emission from the active flare stars EQ Peg, YZ CMi, and AD Leo. No statistically significant evidence for slowly varying emission is found to a level of 0.05 Jy for AD Leo, 0.018-0.021 Jy for YZ CMi, and 0.009-0.018 Jy for EQ Peg. Upper limits of about 10 trillion K are determined for the brightness temperature of active radio regions on these stars at the time of the observations.
Details
- Title: Subtitle
- A search for slowly varying radio continuum emission from UV Ceti stars
- Creators
- S. R SpanglerS. D Shawhan
- Resource Type
- Journal article
- Publication Details
- The Astrophysical journal, Vol.205, p.472
- DOI
- 10.1086/154300
- ISSN
- 0004-637X
- eISSN
- 1538-4357
- Publisher
- University of Chicago Press
- Language
- English
- Date published
- 04/1976
- Academic Unit
- Physics and Astronomy
- Record Identifier
- 9984199772302771
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