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.
Dokumententyp: | Zeitschriftenartikel |
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Fakultät: | Physik |
Themengebiete: | 500 Naturwissenschaften und Mathematik > 530 Physik |
ISSN: | 0094-243X |
Sprache: | Englisch |
Dokumenten ID: | 55793 |
Datum der Veröffentlichung auf Open Access LMU: | 14. Jun. 2018, 10:00 |
Letzte Änderungen: | 04. Nov. 2020, 13:36 |