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Title: Light Curve and SED Modeling of the Gamma-Ray Binary 1FGL J1018.6–5856: Constraints on the Orbital Geometry and Relativistic Flow

Journal Article · · Astrophysical Journal

We present broadband spectral energy distributions and light curves of the gamma-ray binary 1FGL J1018.6−5856 measured in the X-ray and the gamma-ray bands. We find that the orbital modulation in the low-energy gamma-ray band is similar to that in the X-ray band, suggesting a common spectral component. However, above a GeV the orbital light curve changes significantly. We suggest that the GeV band contains significant flux from a pulsar magnetosphere, while the X-ray to TeV light curves are dominated by synchrotron and Compton emission from an intrabinary shock (IBS). We find that a simple one-zone model is inadequate to explain the IBS emission, but that beamed Synchrotron-self Compton radiation from adiabatically accelerated plasma in the shocked pulsar wind can reproduce the complex multiband light curves, including the variable X-ray spike coincident with the gamma-ray maximum. The model requires an inclination of ∼50° and an orbital eccentricity of ∼0.35, consistent with the limited constraints from existing optical observations. This picture motivates searches for pulsations from the energetic young pulsar powering the wind shock.

OSTI ID:
22661184
Journal Information:
Astrophysical Journal, Vol. 838, Issue 2; Other Information: Country of input: International Atomic Energy Agency (IAEA); ISSN 0004-637X
Country of Publication:
United States
Language:
English

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Cited By (6)

Refining the origins of the gamma-ray binary 1FGL J1018.6–5856 journal November 2018
Overview of non-transient γ -ray binaries and prospects for the Cherenkov Telescope Array journal November 2019
Discovery of the Galactic High-Mass Gamma-ray Binary 4FGL J1405.1-6119 collection January 2019
Signatures of Intra-binary Shock Emission in the Black Widow Pulsar Binary PSR J2241−5236 journal November 2018
Discovery of the Galactic High-mass Gamma-Ray Binary 4FGL J1405.1−6119 journal October 2019
Overview of non-transient gamma-ray binaries and prospects for the Cherenkov Telescope Array text January 2019