Very Energetic Gamma-Rays from Microquasars and Binary Pulsars
arXiv:astro-ph/0606393 · doi:10.1126/science.1129815
Abstract
Compact astrophysical objects produce some of the highest energy light in the universe. The challenge is to determine what mechanism produces these photons.
Perspective article to be published in Science vol. 312 (June 23, 2006)
References in corpus (9)
- Sources of Relativistic Jets in the Galaxy
- Variable Very High Energy Gamma-ray Emission from the Microquasar LS I +61 303
- Discovery of the Binary Pulsar PSR B1259-63 in Very-High-Energy Gamma Rays around Periastron with H.E.S.S
- Discovery of very high energy gamma-rays associated with an X-ray binary
- A dark jet dominates the power output of the stellar black hole Cygnus X-1
- Large-Scale, Decelerating, Relativistic X-ray Jets from the Microquasar XTE J1550-654
- A broadband leptonic model for gamma-ray emitting microquasars
- LS 5039: a runaway microquasar ejected from the galactic plane
- A microquasar shot out from its birth place
Cited by in corpus (32)
- High-energy neutrinos in the context of multimessenger physics
- Gamma-ray binaries and related systems
- Modeling interaction of relativistic and nonrelativistic winds in binary system PSR 1259-63/SS2883. I.Hydrodynamical limit
- Accretion vs colliding wind models for the gamma-ray binary LS I +61 303: an assessment
- Periodic Emission from the Gamma-ray Binary 1FGL J1018.6-5856
- A magnetar-like event from LS I +61 303 and its nature as a gamma-ray binary
- Very-high energy gamma-ray astronomy: A 23-year success story in high-energy astroparticle physics
- Revealing Gamma-Ray Binaries
- Pulsar model of the high energy phenomenology of LS 5039
- Relativistic fluid modelling of gamma-ray binaries. I. The model
- Swift/XRT monitoring of five orbital cycles of LSI +61 303
- Relativistic fluid modelling of gamma-ray binaries. II. Application to LS 5039
- High Resolution Radio Astronomy Using Very Long Baseline Interferometry
- Physics of accretion flows around compact objects
- Neutrino signal from gamma-ray loud binaries powered by high energy protons
- High-energy gamma-ray emission from the inner jet of LS I+61 303: the hadronic contribution revisited
- Impact of the orbital uncertainties on the timing of pulsars in binary systems
- Low frequency radio spectrum and spectral turnover of LS 5039
- Astrophysics in 2006
- Dynamical and radiative simulations of -ray jets in microquasars
- Radio emission and jets from microquasars
- Gamma-ray binaries
- Microquasars: summary and outlook
- Orbital and superorbital variability of LS I +61 303 at low radio frequencies with GMRT and LOFAR
- Study of the High Energy Gamma-ray Emission from the Crab Pulsar with the MAGIC telescope and Fermi-LAT
- Black Hole High Mass X-ray Binary Microquasars at Cosmic Dawn
- Results from MAGIC's first observation cycle on galactic sources
- Whipple Telescope Observations of LS I +61 303: 2004-2006
- The Early History of Microquasar Research
- The Supernova Remnant G284.31.8 and Its Relation to the Gamma-ray Binary 1FGL J1018.65856
- H.E.S.S. Observations of LS 5039
- Discovery of microquasar LS I +61 303 at very high energy gamma-rays with MAGIC