X-ray and gamma-ray orbital variability from the gamma-ray binary HESS J1832-093
arXiv:2001.02701 · doi:10.1051/0004-6361/202037442
Abstract
Context. Gamma-ray binaries are systems composed of a massive star and a compact object whose interaction leads to particle acceleration up to relativistic energies. In the last fifteen years, a few binaries have been discovered to emit at high energies, but their number is still scarce. The TeV source HESS J1832-093 has been proposed as a binary candidate, although its nature is unclear. Neither a GeV counterpart nor a period was found for it. Aims. The purpose of this work is to search for a gamma-ray source at GeV energies to understand the origin of the TeV signal. For an unambiguous identification of its binary nature, finding an orbital modulation is crucial. Methods. We have analysed data spanning more than 10 years from the Fermi Large Area Telescope (Fermi-LAT), together with Swift archival observations taken between 2015 and 2018, using both the X-Ray Telescope (XRT) and UltraViolet and Optical Telescope (UVOT). We searched for periodicities in both X-ray and gamma-ray bands using a Lomb-Scargle periodogram. Results. We find a periodic modulation of \sim 86 days in the X-ray source XMMU J183245-0921539, together with indications of gamma-ray modulation with a compatible period in 4FGL J1832.9-0913. Neither an optical nor an UV counterpart is found at the X-ray source location. The overall spectral energy distribution strongly resembles the known gamma-ray binary HESS J0632+057. Conclusions. Both the spectrum and the discovery of an orbital period allow the identification of the TeV source HESS J1832-093 as a new member of the gamma-ray binary class.
arXiv comment9 pages, 9 figures. Accepted by A&A
References in corpus (46)
- Astropy: A Community Python Package for Astronomy
- The Gaia mission
- The Large Area Telescope on the Fermi Gamma-ray Space Telescope Mission
- Binary companions of evolved stars in APOGEE DR14: Search method and catalog of ~5,000 companions
- The Swift X-ray Telescope
- The Swift Ultra-Violet/Optical Telescope
- The Burst Alert Telescope (BAT) on the Swift MIDEX Mission
- Fermi Large Area Telescope Fourth Source Catalog
- Understanding the Lomb-Scargle Periodogram
- TEMPO2, a new pulsar timing package. I: Overview
- The Second Fermi Large Area Telescope Catalog of Gamma-ray Pulsars
- Calibration of X-ray absorption in our Galaxy
- Tempo2, a new pulsar timing package. II: The timing model and precision estimates
- Studies in Astronomical Time Series Analysis. VI. Bayesian Block Representations
- The First Fermi Large Area Telescope Catalog of Gamma-ray Pulsars
- The H.E.S.S. Galactic plane survey
- Variable Very High Energy Gamma-ray Emission from the Microquasar LS I +61 303
- Assessing statistical significance of periodogram peaks
- Discovery of the Binary Pulsar PSR B1259-63 in Very-High-Energy Gamma Rays around Periastron with H.E.S.S
- Gamma-ray binaries and related systems
- The 1st Fermi Lat Supernova Remnant Catalog
- 3.9 day orbital modulation in the TeV gamma-ray flux and spectrum from the X-ray binary LS 5039
- Precise Gamma-Ray Timing and Radio Observations of 17 Fermi Gamma-Ray Pulsars
- Discovery of a point-like very-high-energy gamma-ray source in Monoceros
- HESS J0632+057 : A new gamma-ray binary?
- Periodic Emission from the Gamma-ray Binary 1FGL J1018.6-5856
- Long-term monitoring of the high-energy gamma-ray emission from LS I +61° 303 and LS 5039
- A New TeV Binary: The Discovery of an Orbital Period in HESS J0632+057
- Modelling the high-energy emission from gamma-ray binaries using numerical relativistic hydrodynamics
- Periastron Observations of TeV Gamma-Ray Emission from a Binary System with a 50-year Period
- A Luminous Gamma-ray Binary in the Large Magellanic Cloud
- Timing Gamma-ray Pulsars with the Fermi Large Area Telescope: Timing Noise and Astrometry
- Unraveling the high-energy emission components of gamma-ray binaries
- Long-term TeV and X-ray Observations of the Gamma-ray Binary HESS J0632+057
- Revealing the extended radio emission from the gamma-ray binary HESS J0632+057
- Discovery of the Galactic High-Mass Gamma-ray Binary 4FGL J1405.1-6119
- The first catalog of Fermi-LAT sources below 100 MeV
- Sizing up the population of gamma-ray binaries
- GeV detection of HESS J0632+057
- Discovery of a variable X-ray counterpart to HESS J1832-093: A new gamma-ray binary?
- A hydrodynamics-informed, radiation model for HESS J0632057 from radio to gamma rays
- Interaction Between Supernova Remnant G22.7-0.2 And The Ambient Molecular Clouds
- Investigation of the energy dependence of the orbital light curve in LS 5039
- The missing GeV γ-ray binary: Searching for HESS J0632+057 with Fermi-LAT
- Swift observations of 1FGL J1018.6-5856
- NuSTAR Hard X-ray Observation of the Gamma-ray Binary Candidate HESS J1832-093
Cited by in corpus (8)
- Incremental Fermi Large Area Telescope Fourth Source Catalog
- Advances in Understanding High-Mass X-ray Binaries with INTEGRAL and Future Directions
- Relativistic fluid modelling of gamma-ray binaries. I. The model
- Observation of the gamma-ray binary HESS J0632+057 with the H.E.S.S., MAGIC, and VERITAS telescopes
- Prospects for a survey of the Galactic plane with the Cherenkov Telescope Array
- A multi-wavelength study of the gamma-ray binary candidate HESS J1832-093
- Possible TeV -ray binary origin of HESS J1828-099
- Polarization study of gamma-ray binary