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相关论文: Limits from rapid TeV variability of Mrk 421

200 篇论文

We discuss the correlation between the evolution of the TeV emission and X-ray radiation observed in high-energy peaked BL Lac objects. We describe such a correlation by a simple power law. In the first part of this work we present…

天体物理学 · 物理学 2009-11-10 K. Katarzynski , G. Ghisellini , F. Tavecchio , L. Maraschi , G. Fossati , A. Mastichiadis

In the recent years, the new generation of Imaging Atmospheric Cerenkov Telescopes successfully detected very high energy (VHE; E>100 GeV) gamma-ray emission from a growing number of Active Galactic Nuclei (AGNs), mainly belonging to the…

高能天体物理现象 · 物理学 2009-07-13 J. -P. Lenain

A fraction of AGN producing VHE gamma-rays are located in galaxy clusters. The magnetic field present in the intra-cluster medium would lead to conversions of VHE photons into axion-like particles (ALPs), which are a generic prediction of…

高能天体物理现象 · 物理学 2015-06-05 Dieter Horns , Luca Maccione , Manuel Meyer , Alessandro Mirizzi , Daniele Montanino , Marco Roncadelli

The Large High Altitude Air Shower Observatory recently detected TeV emission from the low-luminosity active galactic nucleus (LLAGN) NGC 4278. Integral-field spectroscopy with MEGARA revealed ionized outflows on hundred-parsec scales with…

高能天体物理现象 · 物理学 2025-09-10 Alberto Domínguez

We observed the BL Lac object Markarian 421 with the X-ray satellite RXTE and the Whipple Air Cerenkov Telescope during a two week correlated X-ray/gamma-ray campaign in May 1996. Two dramatic outbursts with extremely rapid and strong flux…

天体物理学 · 物理学 2009-10-30 Michael Schubnell

We analyze four extreme active galactic nuclei (AGN) transients to explore the possibility that they are caused by rare, high-amplitude microlensing events. These previously unknown type-I AGN are located in the redshift range 0.6-1.1 and…

Gamma-ray bursts (GRB) are generally believed to be efficient particle accelerators. In the presence of energetic protons in a GRB jet, interactions between these protons and intense radiation field of the GRB are supposed to induce…

高能天体物理现象 · 物理学 2023-02-01 Ruo-Yu Liu , Hai-Ming Zhang , Xiang-Yu Wang

Imaging Atmospheric Cherenkov Telescopes (IACTs) allow us to observe Active Galactic Nuclei (AGNs) in the 100 GeV to 20 TeV energy range with high sensitivity. The TeV gamma-ray observations of the nine blazars detected so far in this…

天体物理学 · 物理学 2008-11-26 Henric Krawczynski

The recent Cherenkov telescope observations and detections of the BL Lac objects Mkn 421, Mkn 501, 1ES 2344+514, PKS 2155--304 and possibly 1ES 1959+658 have shown that there exists a subclass of BL Lac objects emitting a substantial…

天体物理学 · 物理学 2009-10-31 Gabriele Ghisellini

We explore several models which might be proposed to explain recent possible detections of high-energy (TeV) gamma rays in association with low-energy gamma-ray bursts (GRBs). Likely values (and/or upper limits) for the source energies in…

天体物理学 · 物理学 2009-11-07 P. C. Fragile , G. J. Mathews , J. Poirier , T. Totani

We present the results from the timing and spectral study of Mrk\,421 based mainly on the \emph{Swift} data in the X-ray energy range obtained during the time interval 2015\,December--2018\,April. The most extreme X-ray flaring activity on…

星系天体物理 · 物理学 2020-04-03 B. Kapanadze , A. Gurchumelia , D. Dorner , S. Vercellone , P. Romano , P. Hughes , M. Aller , H. Aller , O. Kharshiladze

Models with extra dimensions and the fundamental scale at the TeV could imply sign als in large neutrino telescopes due to gravitational scattering of cosmogenic neu trinos in the detection volume. Apart from the production of microscopic…

高能物理 - 唯象学 · 物理学 2007-05-23 J. I. Illana , M. Masip , D. Meloni

The IceCube neutrino telescope has provided upper limits on neutrino emission from gamma ray bursts. These constraints provided by the IceCube detector have been instrumental in investigating the properties of the GRB jet and its emission…

高能天体物理现象 · 物理学 2026-02-16 Chiranjeet Pradhan , Khushboo Sharma , Abhijit Roy , Jagdish C. Joshi

We investigate the production of magnetic flux from rotating black holes in active galactic nuclei (AGNs) and compare it with the upper limit of ultrahigh energy cosmic ray (UHECR) luminosities, calculated from observed integral flux of…

高能天体物理现象 · 物理学 2015-11-04 C. H. Coimbra-Araújo , R. C. Anjos

Over the past decade, our knowledge of the \gamma-ray sky has been revolutionized by ground- and space-based observatories by detecting photons up to several hundreds of tera-electron volt (TeV) energies. A major population of the…

高能天体物理现象 · 物理学 2018-11-05 B. Rani

A wide-frequency radio study of Active Galactic Nuclei (AGN) is crucial to evaluate the intervening radiative mechanisms responsible for the observed emission and relate them with the underlying accretion physics. We present wide frequency…

Sub-photospheric internal shocks and transverse differences of the bulk Lorentz factor in relativistic fireball models of GRB lead to neutron diffusion relative to protons, resulting in inelastic nuclear collisions. This produces…

天体物理学 · 物理学 2009-10-31 P. Meszaros , M. J. Rees

Highly variable Markarian 421 is a bright high synchrotron energy peaked blazar showing wide featureless non-thermal spectrum making it a good candidate for our study of intraday flux and spectral variations over time. We analyse its X-ray…

高能天体物理现象 · 物理学 2024-11-07 A Priyana Noel , Haritma Gaur , Alok C. Gupta , Alicja Wierzcholska , Michal Ostrowski , Vinit Dhiman , Gopal Bhatta

Most active galactic nuclei (AGN) lack prominent jets, and show modest radio emission and significant X-ray emission which arises mainly from the galactic core, very near from the central black hole. We use a quantitative scenario of such…

天体物理学 · 物理学 2009-11-10 Jaime Alvarez-Muñiz , Peter Meszaros

M87 is a nearby radio galaxy that has been detected at energies ranging from radio to very high energy (VHE) gamma-rays. Its proximity and its jet, misaligned from the line of sight allow detailed morphological studies. The imaging…

高能天体物理现象 · 物理学 2015-05-29 Stephane Vincent