Light Curve and SED Modeling of the Gamma-Ray Binary 1FGL J1018.6–5856: Constraints on the Orbital Geometry and Relativistic Flow
Author:
Publisher
American Astronomical Society
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://stacks.iop.org/0004-637X/838/i=2/a=145/pdf
Reference32 articles.
1. THE SECOND FERMI LARGE AREA TELESCOPE CATALOG OF GAMMA-RAY PULSARS
2. Discovery of variable VHEγ-ray emission from the binary system 1FGL J1018.6–5856
3. FERMI LARGE AREA TELESCOPE THIRD SOURCE CATALOG
4. DEVELOPMENT OF THE MODEL OF GALACTIC INTERSTELLAR EMISSION FOR STANDARD POINT-SOURCE ANALYSIS OF FERMI LARGE AREA TELESCOPE DATA
5. Periodic Emission from the Gamma-Ray Binary 1FGL J1018.6–5856
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1. Modeling X-Ray and Gamma-Ray Emission from Redback Pulsar Binaries;The Astrophysical Journal;2024-03-21
2. The high energy X-ray probe (HEX-P): Galactic PeVatrons, star clusters, superbubbles, microquasar jets, and gamma-ray binaries;Frontiers in Astronomy and Space Sciences;2023-12-22
3. Investigation of the Broadband Emission of the Gamma-Ray Binary HESS J0632+057 Using an Intrabinary Shock Model;The Astrophysical Journal;2022-08-29
4. Improved binary solution for the gamma-ray binary 1FGL J1018.6-5856;Monthly Notices of the Royal Astronomical Society;2022-06-27
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