Astronomy and Astrophysics – Astronomy
Scientific paper
Dec 1998
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998aas...193.4313g&link_type=abstract
American Astronomical Society, 193rd AAS Meeting, #43.13; Bulletin of the American Astronomical Society, Vol. 30, p.1315
Astronomy and Astrophysics
Astronomy
Scientific paper
A Bayesian analysis of the phase variations of the 26.5 day periodic radio outbursts from the high mass X-ray binary LSI+61(0) 303 demonstrates a clear periodic modulation on a time scale similar to that previously found for the long term modulation of the outburst peak flux density. Combining the outburst phase and flux information we obtain a phase and flux modulation period of 1584_{-11}(+14) days as well as a more accurate outburst period of 26.4917 +/- .0025 days. From the shape of the phase and outbursts flux modulation we find that larger outbursts occur at an earlier orbital phase, closer to periastron, probably as a result of variations in the wind from the rapidly rotating B star primary. The next maximum in long term flux modulation is predicted to occur between February, 1999 and March, 2000 (Julian day 2,451,233 to 2,451,633).
Gregory Philip C.
Peracaula Marta
Taylor Russ A.
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