RADIO-EMISSION OF YZ CMI AT 1.6, 2 AND 3.6 CM

Authors
Citation
Sm. Rucinski, RADIO-EMISSION OF YZ CMI AT 1.6, 2 AND 3.6 CM, Acta Astronomica, 44(1), 1994, pp. 75-79
Citations number
11
Categorie Soggetti
Astronomy & Astrophysics
Journal title
ISSN journal
00015237
Volume
44
Issue
1
Year of publication
1994
Pages
75 - 79
Database
ISI
SICI code
0001-5237(1994)44:1<75:ROYCA1>2.0.ZU;2-G
Abstract
Observations at two epochs at the currently shortest wavelengths acces sible with the VLA1 system are presented. YZ CMi was observed to be su rprisingly radio bright at these wavelengths which, taken together wit h previous 6 - 20 cm observations and variability between the epochs, suggests non-thermal origin of electrons producing the gyrosynchrotron emission.