Abstract
The high-mass X-ray binary LS I + 61 degrees 303 is detected from radio up to very high energy gamma-rays. The source consists of a Be star and a compact object in an eccentric orbit. Observations have shown evidence for radio microflares superimposed on larger outbursts. We observed the decaying phase of one large radio outburst with the 100-m telescope in Effelsberg at 5, 8, and 10 GHz. We observed microflaring activity with periodicities of 9.5 and 14.9 hours. We discuss the possible physical processes behind these quasi-periodic oscillations.
Item Type: | Journal article |
---|---|
Faculties: | Physics |
Subjects: | 500 Science > 530 Physics |
ISSN: | 0094-243X |
Language: | English |
Item ID: | 55793 |
Date Deposited: | 14. Jun 2018, 10:00 |
Last Modified: | 04. Nov 2020, 13:36 |