Overview of non-transient gamma-ray binaries and prospects for the Cherenkov Telescope Array
arXiv:1909.11018 · doi:10.1051/0004-6361/201936501
Abstract
We simulate the spectral behaviour of the non-transient gamma-ray binaries using archival observations as a reference. With this we test the CTA capability to measure the sources' spectral parameters and detect variability on various time scales. We review the known properties of gamma-ray binaries and the theoretical models that have been used to describe their spectral and timing characteristics. We show that CTA is capable of studying these sources on time scales comparable to their characteristic variability time scales. For most of the binaries, the unprecedented sensitivity of CTA will allow the spectral evolution to be studied on a time scale as short as 30 min. This will enable a direct comparison of the TeV and lower energy (radio to GeV) properties of these sources from simultaneous observations. We also review the source-specific questions that can be addressed with such high-accuracy CTA measurements.
Accepted to A&A
References in corpus (50)
- Observations of the Crab Nebula with H.E.S.S
- An eclipsing binary distance to the Large Magellanic Cloud accurate to 2 per cent
- Discovery of High-Energy Gamma-Ray Emission from the Binary System PSR B1259-63/LS 2883 Around Periastron with Fermi
- VERITAS Observations of the gamma-Ray Binary LS I +61 303
- On the formation of TeV radiation in LS 5039
- TeV lightcurve of PSR B1259-63/SS2883
- Discovery of a point-like very-high-energy gamma-ray source in Monoceros
- Detection of Gamma-ray Emission from the Eta-Carinae Region
- HESS J0632+057 : A new gamma-ray binary?
- Periodic very high energy gamma-ray emission from LS I +61 303 observed with the MAGIC telescope
- Periodic Emission from the Gamma-ray Binary 1FGL J1018.6-5856
- γ^2 Velorum: Orbital Solution and Fundamental Parameter Determination with SUSI
- GammaLib and ctools: A software framework for the analysis of astronomical gamma-ray data
- Multiwavelength monitoring and X-ray brightening of Be X-ray binary PSR J2032+4127/MT91 213 on its approach to periastron
- The modulation of the gamma-ray emission from the binary LS 5039
- Modeling the RXTE light curve of Carinae from a 3-D SPH simulation of its binary wind collision
- A Luminous Gamma-ray Binary in the Large Magellanic Cloud
- Unraveling the high-energy emission components of gamma-ray binaries
- XMM-Newton observation of a spectral state transition in the peculiar radio/X-ray/gamma-ray source LS I +61 303
- Hard X-ray emission from Eta Carinae
- Detection of persistent gamma-ray emission toward SS433/W50
- Gamma-ray follow-up studies on Eta Carinae
- Hadronic model for radio-to-TeV gamma-ray emission from PSR B1259-63
- Superorbital modulation of X-ray emission from gamma-ray binary LSI +61 303
- A close encounter of the massive kind
- Sizing up the population of gamma-ray binaries
- Long-term periodicity in LSI+61303 as beat frequency between orbital and precessional rate
- High-energy observations of PSR B1259-63/LS 2883 through the 2014 periastron passage: connecting X-rays to the GeV flare
- Overview of non-transient gamma-ray binaries and prospects for the Cherenkov Telescope Array
- Discovery of the VHE gamma-ray source HESS J1832-093 in the vicinity of SNR G22.7-0.2
- On the origin of γ-ray emission in η Carina
- GeV detection of HESS J0632+057
- Simulations of an inhomogeneous stellar wind interacting with a pulsar wind in a binary system
- Carinae Baby Homunculus Uncovered by ALMA
- Study of orbital and superorbital variability of LSI +61 303 with X-ray data
- Investigation of the energy dependence of the orbital light curve in LS 5039
- 3D magneto-hydrodynamic models of non-thermal photon emission in the binary system Velorum
- Probing the nature of the TeV gamma-ray binary HESS J0632+057 by monitoring Be disk variability
- The orbital parameters of the gamma-ray binary LMC P3
- Discovery of a periodical apoastron GeV peak in LS I +61°303
- Electron-positron pair production by gamma rays in an anisotropic flux of soft photons, and application to pulsar polar caps
- Long-term OVRO monitoring of LSI+61303: confirmation of the two close periodicities
- The gamma-ray source AGL J2241+4454 as the possible counterpart of MWC 656
- A rotating hollow cone anisotropy of TeV emission from binary systems
- Gamma-gamma absorption in the -ray binary system PSR B1259-63/LS 2883
- Ambient magnetic field amplification in shock fronts of relativistic jets: an application to GRB afterglows
- The orbit of the gamma-ray binary 1FGL J1018.6-5856
- NuSTAR Hard X-ray Observation of the Gamma-ray Binary Candidate HESS J1832-093
- Peculiar objects towards 3FGL J0133.3+5930: an eclipsing Be star and an active galactic nucleus
- Phenomenology of gamma-ray emitting binaries
Cited by in corpus (10)
- ASTRI Mini-Array Core Science at the Observatorio del Teide
- New insight into the origin of the GeV flare in the binary system PSR B1259-63 from the 2017 periastron passage
- Overview of non-transient gamma-ray binaries and prospects for the Cherenkov Telescope Array
- Multi-wavelength observations of PSRJ 2032+4127 during the 2017 periastron passage
- Prospects for a survey of the Galactic plane with the Cherenkov Telescope Array
- NuSTAR and XMM-Newton observations of the binary 4FGL J1405.1-6119. A -ray emitting microquasar?
- Improved binary solution for the gamma-ray binary 1FGL J1018.6-5856
- Galactic transient sources with the Cherenkov Telescope Array Observatory
- Radio counterparts of gamma-ray sources in the Cygnus region
- Colliding-Wind Binaries as a Source of TeV Cosmic Rays