Connection between orbital modulation of H-alpha and gamma-rays in the Be/X-ray binary LSI+61303
arXiv:1311.7618 · doi:10.1051/0004-6361/201322936
Abstract
We studied the average orbital modulation of various parameters (gamma-ray flux, H-alpha emission line, optical V band brightness) of the radio- and gamma-ray emitting Be/X-ray binary LSI+61303. Using the Spearman rank correlation test, we found highly significant correlations between the orbital variability of the equivalent width of the blue hump of the H-alpha and Fermi-LAT flux with a Spearman p-value 2e-5, and the equivalent widths ratio EW_B/EW_R and Fermi-LAT flux with p-value 9e-5. We also found a significant anti-correlation between Fermi-LAT flux and V band magnitude with p-value 7.10^{-4}. All these correlations refer to the average orbital variability, and we conclude that the H-alpha and gamma-ray emission processes in LSI+61303 are connected. The possible physical scenario is briefly discussed.
accepted as a Letter in Astronomy and Astrophysics
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- Optical and Near-Infrared Monitoring of Gamma-ray Binaries Hosting Be Stars
- Achromatic rapid flares in hard X-rays in the -ray binary LS I +61-303
- Optical microflares in LS I +61 303 and the search for their multiwavelength counterpart