中文
相关论文

相关论文: Probing orbital parameters of gamma-ray binaries w…

200 篇论文

Gamma-ray binaries are orbital modulated gamma-ray sources in the Galaxy detected both at GeV and TeV energies. The high-energy radiation may come from the interaction of energetic electrons injected by a young pulsar and photons from the…

高能天体物理现象 · 物理学 2009-12-21 B. Cerutti , G. Dubus , G. Henri

The population of binary systems known to emit in the GeV and TeV bands consists of only a few firmly identified Galactic sources. These rare objects constitute extreme particle accelerators operating under varying, but regularly repeating,…

高能天体物理现象 · 物理学 2009-12-25 J. Holder

Gamma-ray binaries are thought to be composed of a young pulsar in orbit around a massive O or Be star, with their gamma-ray emission powered by pulsar spindown. The number of such systems in our Galaxy is not known. We aim to estimate the…

高能天体物理现象 · 物理学 2017-12-13 Guillaume Dubus , Nicolas Guillard , Pierre-Olivier Petrucci , Pierrick Martin

During last years a few massive binary systems have been detected in the TeV gamma-rays. This gamma-ray emission is clearly modulated with the orbital periods of these binaries suggesting its origin inside the binary system. In this paper…

天体物理学 · 物理学 2008-06-27 W. Bednarek

Gamma-ray emission in the TeV range has been detected by HESS from two X-ray binaries: PSR B1259-63 and LS 5039. In both, the early-type star provides large numbers of target photons for pair-production with TeV gamma-rays. This results in…

天体物理学 · 物理学 2009-11-11 Guillaume Dubus

Gamma-ray binaries are a subclass of high-mass binary systems whose energy spectrum peaks at high energies (E$\gtrsim$100 MeV) and extends to very high energies (E$\gtrsim$100 GeV) $\gamma$ rays. In this review we summarize properties of…

高能天体物理现象 · 物理学 2020-06-09 Maria Chernyakova , Denys Malyshev

Several binary systems consisting of a massive star and a compact object have been detected above 100 GeV in the Galaxy. In most of these sources, gamma-rays show a modulation associated to the orbital motion, which means that the emitter…

高能天体物理现象 · 物理学 2015-05-18 V. Bosch-Ramon

Gamma-ray binaries are suitable sources to study high-energy processes in jets and outflows in general. In the last years, there has been a lot of activity in the field of gamma-ray binaries to identify the different factors that shape…

高能天体物理现象 · 物理学 2010-08-04 V. Bosch-Ramon

A long standing problem in high energy astrophysics is the nature of galactic accelerators of particles with energies above PeV. Such objects are sources of galactic cosmic rays and can produce PeV-regime photons observed by ground-based…

高能天体物理现象 · 物理学 2026-03-16 A. M. Bykov , A. E. Petrov , K. P. Levenfish

Gamma-ray binaries are systems composed of a compact object orbiting a massive companion star. The interaction between these two objects can drive relativistic outflows, either jets or winds, in which particles can be accelerated to…

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…

高能天体物理现象 · 物理学 2020-05-06 G. Martí-Devesa , O. Reimer

At least one massive binary system containing an energetic pulsar, PSR B1259-63/SS2883, has been recently detected in the TeV gamma-rays by the HESS telescopes. These gamma-rays are likely produced by particles accelerated in the vicinity…

天体物理学 · 物理学 2009-11-13 Agnieszka Sierpowska-Bartosik , Wlodek Bednarek

After initial claims and a long hiatus, it is now established that several binary stars emit high (0.1-100 GeV) and very high energy (>100 GeV) gamma rays. A new class has emerged called 'gamma-ray binaries', since most of their radiated…

高能天体物理现象 · 物理学 2013-09-06 Guillaume Dubus

It is at present well known that conditions at some massive binary systems allow acceleration of particles and production of the GeV-TeV gamma-rays. However, which particles are responsible for this emission and what radiation processes are…

高能天体物理现象 · 物理学 2015-06-03 W. Bednarek

We consider propagation of very high energy (VHE) gamma-rays in the radiation field of a massive star in the binary system Cen X-3, which has been reported as a source of gamma-ray photons in the GeV and TeV energies. VHE gamma-rays or…

天体物理学 · 物理学 2011-05-23 W. Bednarek

The production site of gamma rays in blazars is closely related to their interaction with the photon fields surrounding the active galactic nucleus. In this paper, we discuss an indirect method that may help to unveil the presence of…

高能天体物理现象 · 物理学 2022-02-21 L. Foffano , V. Vittorini , M. Tavani , E. Menegoni

Compact binary systems can provide us with unique information on astrophysical particle acceleration and cosmic ray production. However, only five binary systems have ever been observed in TeV $\gamma$ rays. The High Altitude Water…

高能天体物理现象 · 物理学 2017-08-15 Chang Dong Rho

Gamma-ray binaries are X-ray binaries with gamma-ray emissions. Their multi-wavelength emissions range from radio, optical, X-ray and to very high energy (TeV). X-ray emissions are crucial to understand the nature of gamma-ray binaries.…

高能天体物理现象 · 物理学 2013-02-22 Jian Li , Diego F. Torres , Shu Zhang , Jianmin Wang

The Milky Way contains hundreds of binary systems which are known to emit in radio and X-rays, but only a handful of binaries have been observed to produce very high-energy gamma rays. In addition, the emission mechanisms which produce the…

高能天体物理现象 · 物理学 2019-08-13 Segev BenZvi

Recent ground based and space telescopes that detect high energy photons from a few up to hundreds of gigaelectron volts (GeV) have opened a new window on the universe. However, because of the relatively poor angular resolution of these…

高能天体物理现象 · 物理学 2015-06-03 I. F. Mirabel
‹ 上一页 1 2 3 10 下一页 ›