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 |
|---|---|
| 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 |
