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LS I +61$^\circ$ ~303 is one of around ten gamma-ray binaries detected so far which has a spectral energy distribution dominated by MeV-GeV photons. It is located at a distance of 2 kpc and consists of a compact object (black hole or…

High Energy Astrophysical Phenomena · Physics 2021-08-23 D. B. Kieda

We present the results of a multiwavelength monitoring campaign targeting the gamma-ray source 2CG 135+1 in an attempt to confirm the association of this object with the radio/Be/X-ray binary system LSI +61o 303. The campaign included…

Astrophysics · Physics 2009-10-30 M. S. Strickman , M. Tavani , M. J. Coe , I. A. Steele , J. Fabregat , J. Marti , J. M. Paredes , P. S. Ray

Type III bursts and hard X-rays are both produced by flare energetic electron beams. The link between both emissions has been investigated in many previous studies, but no statistical studies have compared both coronal and interplanetary…

Solar and Stellar Astrophysics · Physics 2017-01-04 Hamish A. S. Reid , Nicole Vilmer

In this paper, the correlation between the gamma-ray and the radio bands is investigated. The results show that there is a closer correlation between the gamma-ray emission and the high frequency (1.3mm, 230GHz) radio emission for maximum…

Astrophysics · Physics 2007-05-23 J. H. Fan , G. Adam , G. Z. Xie , S. L. Cao , R. G. Lin , Y. Copin

We present the results from simultaneous radio (Very Large Array) and X-ray (Rossi-X-ray Timing Explorer) observations of the Z-type neutron star X-ray binary GX~17+2. The aim is to assess the coupling between X-ray and radio properties…

Cygnus X-3, among the Galactic X-ray binaries, is one of the brightest radio sources. Radio image as well as spectral analysis shows the presence of outflow in the form of jets. The SED in the X-ray band shows a complicated structure and…

Astrophysics · Physics 2007-05-23 M. Choudhury , A. R. Rao

Context. A short duration burst reminiscent of a soft gamma-ray repeater/anomalous X-ray pulsar behaviour was detected in the direction of LS I +61 303 by the Swift satellite. While the association with this well known gamma-ray binary is…

High Energy Astrophysical Phenomena · Physics 2009-11-13 A. J. Munoz-Arjonilla , J. Marti , J. A. Combi , P. Luque-Escamilla , J. R. Sanchez-Sutil , V. Zabalza , J. M. Paredes

Long time scale radio-X-ray correlations in black holes during the hard state have been found in many sources and there seems to emerge a universal underlying relationship which quantitatively describes this behavior. Although it would…

One of the most enigmatic TeV binary systems, LS I +61$^\circ$ 303 exhibits a high degree of flux modulation from radio to TeV wavelengths over a single orbit of the binary system, once every $\sim$26.5 days. The binary system also exhibits…

High Energy Astrophysical Phenomena · Physics 2019-08-17 Payel Kar

LSI +61 303 is one of the few X-ray binaries with a Be star companion from which radio, X-rays and high-energy gamma-ray (GeV and TeV) emission have been observed. The nature of the high energy activity of the system is not yet fully…

High Energy Astrophysical Phenomena · Physics 2017-07-19 M. Chernyakova , Iu. Babyk , D. Malyshev , Ie. Vovk , S. Tsygankov , H. Takahashi , Ya. Fukazawa

We present the results of a detailed correlation study between the soft X-ray, hard X-ray, and radio emission (obtained from RXTE ASM, BATSE, and GBI observations, respectively) of the bright radio emitting Galactic X-ray binary Cygnus X-3.…

Astrophysics · Physics 2009-11-07 M. Choudhury , A. R. Rao , S. V. Vadawale , C. H. Ishwara-Chandra , A. K. Jain

We present the results of the correlation between the nuclear 2-10 keV X-ray and radio (at 2cm, 6cm and 20cm) luminosities for a well defined sample of local Seyfert galaxies. We use a sample of low luminosity radio galaxies (LLRGs) for…

Astrophysics · Physics 2009-11-13 F. Panessa , X. Barcons , L. Bassani , M. Cappi , F. J. Carrera , L. C. Ho , S. Pellegrini

The gamma-ray binary LS I +61 303 is composed of a Be star and a compact companion orbiting in an eccentric orbit. Variable flux modulated with the orbital period of ~26.5 d has been detected from radio to very high-energy gamma rays. In…

High Energy Astrophysical Phenomena · Physics 2015-02-25 X. Paredes-Fortuny , M. Ribó , V. Bosch-Ramon , J. Casares , O. Fors , J. Núñez

In order to determine the location of the gamma-ray emission site in blazars, we investigate the time-domain relationship between their radio and gamma-ray emission. Light-curves for the brightest detected blazars from the first 3 years of…

Since mid-2007 we have carried out a dedicated long-term monitoring programme at 15 GHz using the Owens Valley Radio Observatory 40 meter telescope. One of the main goals of this programme is to study the relation between the radio and…

High Energy Astrophysical Phenomena · Physics 2015-06-23 W. Max-Moerbeck , J. L. Richards , T. Hovatta , V. Pavlidou , T. J. Pearson , A. C. S. Readhead , O. G. King , R. Reeves

We present INTEGRAL spectral analysis in the orbital/superorbital phase space of LS I +61 303. A hard X-ray spectrum with no cutoff is observed at all orbital/superorbital phases. The hard X-ray index is found to be uncorrelated with the…

High Energy Astrophysical Phenomena · Physics 2015-06-18 Jian Li , Diego F. Torres , Shu Zhang

[Context] The broadband spectral energy distribution of microquasars has proven to be a valuable tool for assessing the roles of jets and accretion flows in microquasars, as well as the coupling between the two. The coupling might manifest…

Astrophysics · Physics 2009-11-13 Yongquan Xue , Wei Cui

This review discusses the complementary relationship between radio and hard X-ray observations of the Sun using primarily results from the era of the Reuven Ramaty High Energy Solar Spectroscopic Imager satellite. A primary focus of joint…

We report on the results of a long term X-ray monitoring campaign of the galactic binary LS I +61 303 performed by the Rossi X-ray Timing Explorer. This dataset consists of 1 ks pointings taken every other day between 2007 August 28 until…

Astrophysics · Physics 2011-02-11 A. Smith , P. Kaaret , J. Holder , A. Falcone , G. Maier , D. Pandel , M. Stroh

LS I +61 303 is one of the most studied X-ray binary systems because of its two peculiarities: On the one hand being the probable counterpart of the variable gamma ray source 2CG 135+01 (Gregory and Taylor 1978; Tavani et al. 1998) and on…

Astrophysics · Physics 2009-11-10 M. Massi , M. Ribo' , J. M. Paredes , S. T. Garrington , M. Peracaula , J. Marti'