activity
19932026
most citedEnergy spectra of gamma-rays, electrons and neutrinos produced at proton-proton interactions in the very high energy regime

924 citations · 39.2k across the 592 of their papers we have counts for

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Showing 2011Show all

28 papers · 1 filter

astro-ph.HE2011★ 23 cited

Galactic Sources of High-Energy Neutrinos: Highlights

Francesco Vissani, Felix Aharonian

We overview high-energy neutrinos from galactic sources, transparent to their gamma-ray emission. We focus on young supernova remnants and in particular on RX J1713.7-3946, discuss…

astro-ph.HE2011★ 29 cited

Simultaneous multi-wavelength campaign on PKS 2005-489 in a high state

The H. E. S. S. Collaboration, the Fermi LAT Collaboration, : +345

The high-frequency peaked BL Lac object PKS 2005-489 was the target of a multi-wavelength campaign with simultaneous observations in the TeV gamma-ray (H.E.S.S.), GeV gamma-ray (Fe…

astro-ph.HE2011★ 116 cited

Discovery of extended VHE γ-ray emission from the vicinity of the young massive stellar cluster Westerlund 1

HESS Collaboration, A. Abramowski, F. Acero +198

Results obtained in very-high-energy (VHE; E > 100 GeV) γ-ray observations performed with the H.E.S.S. telescope array are used to investigate particle acceleration processes in th…

astro-ph.CO2011★ 188 cited

The 2010 very high energy gamma-ray flare & 10 years of multi-wavelength observations of M 87

The H. E. S. S. Collaboration, :, A. Abramowski +442

Abridged: The giant radio galaxy M 87 with its proximity, famous jet, and very massive black hole provides a unique opportunity to investigate the origin of very high energy (VHE;…

astro-ph.GA2011★ 70 cited

X-ray Diagnostics of Giant Molecular Clouds in the Galactic Center Region and Past Activity of Sgr A*

Hirokazu Odaka, Felix Aharonian, Shin Watanabe +3

Strong iron fluorescence at 6.4 keV and hard-X-ray emissions from giant molecular clouds in the Galactic center region have been interpreted as reflections of a past outburst of th…

astro-ph.HE2011★ 27 cited

"Leading blob" model in a stochastic acceleration scenario: the case of the 2009 flare of Mkn~501

E. Lefa, F. A. Aharonian, F. M. Rieger

Evidence for very hard, intrinsic -ray source spectra, as inferred after correction for absorption in the extragalactic background light (EBL), has interesting implications for…

astro-ph.HE2011★ 41 cited

Discovery of the source HESS J1356-645 associated with the young and energetic PSR J1357-6429

HESS Collaboration, A. Abramowski, F. Acero +195

Several newly discovered very-high-energy (VHE; E > 100 GeV) gamma-ray sources in the Galaxy are thought to be associated with energetic pulsars. Among them, middle-aged (> 1E+4 yr…

astro-ph.HE2011★ 53 cited

Modelling interaction of relativistic and non-relativistic winds in binary system PSR B1259-63/SS2883 - II. Impact of magnetization and anisotropy of the pulsar wind

S. Bogovalov, D. Khangulyan, A. V. Koldoba +2

In this paper, we present a numerical study of the properties of the flow produced by the collision of a magnetized anisotropic pulsar wind with its environment in binary system. W…

astro-ph.HE2011★ 72 cited

Post-Periastron Gamma Ray Flare from PSR B1259-63/LS 2883 as a Result of Comptonization of the Cold Pulsar Wind

D. Khangulyan, F. A. Aharonian, S. V. Bogovalov +1

We argue that the bright flare of the binary pulsar \object{PSR B125963/LS2883} detected by the {\it Fermi} Large Area Telescope (LAT), is due to the inverse Compton (IC) scatte…

astro-ph.HE2011★ 76 cited

The need for a local source of UHE CR nuclei

Andrew M. Taylor, Markus Ahlers, Felix A. Aharonian

Recent results of the Pierre Auger (Auger) fluorescence detectors indicate an increasingly heavy composition of ultra-high energy (UHE) cosmic rays (CRs). Assuming that this trend…

astro-ph.HE2011★ 54 cited

Very-high-energy gamma-ray emission from the direction of the Galactic globular cluster Terzan 5

HESS Collaboration, A. Abramowski, F. Acero +194

The H.E.S.S. very-high-energy (VHE, E > 0.1 TeV) gamma-ray telescope system has discovered a new source, HESS J1747-248. The measured integral flux is (1.2 +/- 0.3) \times 10^-12 c…

astro-ph.HE2011★ 124 cited

Formation of hard very-high energy spectra of blazars in leptonic models

E. Lefa, F. M. Rieger, F. Aharonian

The very high energy (VHE) -ray spectra of some TeV Blazars, after being corrected for absorption in the extragalactic background light (EBL), appear unusually hard, which poses…

astro-ph.HE2011★ 29 cited

Modeling the hard TeV spectra of blazars 1ES 0229+200 and 3C 66A with an internal absorption scenario

Olga Zacharopoulou, Dmitry Khangulyan, Felix A. Aharonian +1

We study the applicability of the idea of internal absorption of gamma-rays produced through synchrotron radiation of ultrarelativistic protons in highly magnetized blobs to 1ES 02…

astro-ph.HE2011★ 83 cited

A new SNR with TeV shell-type morphology: HESS J1731-347

HESS Collaboration, A. Abramowski, F. Acero +195

The recent discovery of the radio shell-type supernova remnant (SNR), G353.6-0.7, in spatial coincidence with the unidentified TeV source HESS J1731-347 has motivated further obser…

gr-qc2011★ 2 cited

Mechanics and kinetics in the Friedmann-Lemaitre-Robertson-Walker space-times

S. R. Kelner, A. Yu. Prosekin, F. A. Aharonian

Using the standard canonical formalism, the equations of mechanics and kinetics in the Friedmann-Lemaitre-Robertson-Walker (FLRW) space-times in Cartesian coordinates have been obt…

astro-ph.HE2011★ 4 cited

Non-variable cosmologically distant gamma-ray emitters as an imprint of propagation of ultra-high-energy protons

A. Yu. Prosekin, S. R. Kelner, F. A. Aharonian

The acceleration cites of ultra-high-energy (UHE) protons can be traced by the footprint left by these particles propagating through cosmic microwave background (CMB) radiation. Se…

astro-ph.HE2011★ 55 cited

GRIPS - Gamma-Ray Imaging, Polarimetry and Spectroscopy

J. Greiner, K. Mannheim, F. Aharonian +65

We propose to perform a continuously scanning all-sky survey from 200 keV to 80 MeV achieving a sensitivity which is better by a factor of 40 or more compared to the previous missi…

astro-ph.HE2011★ 49 cited

Cosmic rays in galactic and extragalactic magnetic fields

Felix Aharonian, Andrei Bykov, Etienne Parizot +2

We briefly review sources of cosmic rays, their composition and spectra as well as their propagation in the galactic and extragalactic magnetic fields, both regular and fluctuating…

astro-ph.HE2011★ 47 cited

H.E.S.S. observations of the globular clusters NGC 6388 and M 15 and search for a Dark Matter signal

HESS Collaboration, A. Abramowski, F. Acero +195

Observations of the globular clusters NGC 6388 and M 15 were carried out by the H.E.S.S. array of Cherenkov telescopes for a live time of 27.2 and 15.2 hours respectively. No gamma…

astro-ph.HE2011

Molecular Clouds as Cosmic Ray Laboratories

Sabrina Casanova, Felix A. Aharonian, Yasuo Fukui +9

We will here discuss how the gamma-ray emission from molecular clouds can be used to probe the cosmic ray flux in distant regions of the Galaxy and to constrain the highly unknown…

astro-ph.HE2011★ 26 cited

Gamma Ray Signal from the Pulsar Wind in the Binary Pulsar system PSR B1259-63/LS2883

Dmitry Khangulyan, Felix Aharonian, Sergey Bogovalov +1

Binary pulsar systems emit potentially detectable components of gamma ray emission due to Comptonization of the optical radiation of the companion star by relativistic electrons of…

astro-ph.HE2011★ 126 cited

Astrophysical parameters of LS2883 and implications for the PSR B1259-63 gamma-ray binary

Ignacio Negueruela, Marc Ribó, Artemio Herrero +3

Only a few binary systems with compact objects display TeV emission. The physical properties of the companion stars represent basic input to understand the physical mechanisms behi…

astro-ph.HE2011★ 270 cited

Search for a Dark Matter annihilation signal from the Galactic Center halo with H.E.S.S

H. E. S. S. Collaboration, :, A. Abramowski +193

A search for a very-high-energy (VHE; >= 100 GeV) gamma-ray signal from self-annihilating particle Dark Matter (DM) is performed towards a region of projected distance r ~ 45-150 p…

astro-ph.HE2011★ 39 cited

HESS J1943+213: a candidate extreme BL Lacertae object

H. E. S. S. Collaboration, :, A. Abramowski +200

We report on a newly detected point-like source, HESS J1943+213 located in the Galactic plane. This source coincides with an unidentified hard X-ray source IGR J19443+2117, which w…