A search for slowly varying radio continuum emission from UV Ceti stars

Journal Article · Thu Apr 15 04:00:00 EST 1976 · Astrophys. J.; (United States)

DOI:https://doi.org/10.1086/154300· OSTI ID:7361370

Spangler, S R; Shawhan, S D

A search has been made for a 430 MHz radio counterpart to the optical quiescent variations of flare stars for the stars EQ Peg, YZ CMi, and AD Leo using the Arecibo radiotelescope. No discernible emission was detected. Upper limits of about 0.01, 0.02, and 0.05 janskys were set for the amplitude of this type of emission from EQ Peg, YZ CMi, and AD Leo, respectively. (AIP)

• Research Organization: Department of Physics and Astronomy, The University of Iowa
• OSTI ID: 7361370
• Journal Information: Astrophys. J.; (United States), Journal Name: Astrophys. J.; (United States) Vol. 205:2; ISSN ASJOA
• Country of Publication: United States
• Language: English

Related Subjects

640102* -- Astrophysics & Cosmology-- Stars & Quasi-Stellar
Radio & X-Ray Sources
640103 -- Astrophysics & Cosmology-- Quasi-Stellar
Radio
& X-Ray Sources-- (-1987)
71 CLASSICAL AND QUANTUM MECHANICS
GENERAL PHYSICS
BRIGHTNESS
COSMIC RADIO SOURCES
ELECTROMAGNETIC RADIATION
OPTICAL PROPERTIES
PHYSICAL PROPERTIES
RADIATIONS
RADIOWAVE RADIATION
STARS
STELLAR FLARES
TEMPERATURE DEPENDENCE
VARIABLE STARS
VARIATIONS