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2007ApJ...669..106K - Astrophys. J., 669, 106-108 (2007/November-1)

Confirmation of the 62 day X-ray periodicity from M 82.

KAARET P. and FENG H.

Abstract (from CDS):

Using 400 days of new X-ray monitoring of M82, we confirm the 62 day periodicity previously reported. In the full data set spanning 1124 days, we find a period of 62.0±0.3 days and a coherence, Q=22.3, that is consistent with a strictly periodic signal. We estimate that the probability of chance occurrence of our observed signal is 6x10–7. The light curve folded at this period is roughly sinusoidal and has a peak-to-peak amplitude of (0.99±0.10)x10–11 erg/cm2/s. Confirmation of the periodicity strengthens our previous suggestion that the 62 day modulation is due to orbital motion within an X-ray binary.

Abstract Copyright:

Journal keyword(s): Black Hole Physics - Galaxies: Individual: Messier Number: M82 - Galaxies: Stellar Content - X-Rays: Binaries - X-Rays: Galaxies

Simbad objects: 10

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