activity
20092023
most citedCosmic-ray ionization of molecular clouds

387 citations · 4.6k across the 82 of their papers we have counts for

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Showing astro-ph.HEShow all

36 papers · 1 filter

astro-ph.HE2021★ 24 cited

Spectral index of synchrotron emission: insights from the diffuse and magnetised interstellar medium

Marco Padovani, Andrea Bracco, Vibor Jelić +2

The interpretation of Galactic synchrotron observations is complicated by the degeneracy between the strength of the magnetic field perpendicular to the line of sight (LOS), $B_\pe…

astro-ph.HE2021★ 27 cited

Grammage of cosmic rays in the proximity of supernova remnants embedded in a partially ionized medium

S. Recchia, D. Galli, L. Nava +5

We investigate the damping of Alfvén waves generated by the cosmic ray resonant streaming instability in the context of the cosmic ray escape and propagation in the proximity of su…

astro-ph.HE2021★ 13 cited

The double signature of local cosmic-ray acceleration in star-forming regions

Marco Padovani, Alexandre Marcowith, Daniele Galli +2

Recently, there has been an increased interest in the study of the generation of low-energy cosmic rays (CRs; < 1 TeV) in shocks situated on the surface of a protostar or along pro…

astro-ph.HE2021★ 23 cited

Particle acceleration and magnetic field amplification in massive young stellar object jets

Anabella Araudo, Marco Padovani, Alexandre Marcowith

Synchrotron radio emission from non-relativistic jets powered by massive protostars has been reported, indicating the presence of relativistic electrons and magnetic fields of stre…

astro-ph.HE2020★ 13 cited

Interstellar anatomy of the TeV gamma-ray peak in the IC443 supernova remnant

P. Dell'Ova, A. Gusdorf, M. Gerin +11

Supernovae remnants (SNRs) represent a major feedback source from stars on the interstellar medium of galaxies. During the latest stage of supernovae explosions, shock waves produc…

astro-ph.HE2019★ 36 cited

Non-thermal emission from cosmic rays accelerated in HII regions

M. Padovani, A. Marcowith, Á. Sánchez-Monge +2

Radio observations at metre-centimetre wavelengths shed light on the nature of the emission of HII regions. Usually this category of objects is dominated by thermal radiation produ…

astro-ph.HE2019★ 66 cited

The 2014 TeV Gamma-ray Flare of Mrk 501 Seen with H.E.S.S.: Temporal and Spectral Constraints on Lorentz Invariance Violation

H. E. S. S. Collaboration, :, H. Abdalla +232

The blazar Mrk 501 (z=0.034) was observed at very-high-energy (VHE, ~GeV) gamma-ray wavelengths during a bright flare on the night of 2014 June 23-24 (MJD 56832) with…

astro-ph.HE2018★ 23 cited

Synchrotron emission in molecular cloud cores: the SKA view

Marco Padovani, Daniele Galli

Understanding the role of magnetic fields in star-forming regions is of fundamental importance. In the near future, the exceptional sensitivity of SKA will offer a unique opportuni…

astro-ph.HE2018★ 4 cited

VHE -ray discovery and multi-wavelength study of the blazar 1ES 2322-409

H. E. S. S. Collaboration, :, H. Abdalla +232

A hotspot at a position compatible with the BL Lac object 1ES 2322-409 was serendipitously detected with H.E.S.S. during observations performed in 2004 and 2006 on the blazar PKS 2…

astro-ph.HE2018★ 56 cited

Searches for gamma-ray lines and `pure WIMP' spectra from Dark Matter annihilations in dwarf galaxies with H.E.S.S

H. E. S. S. Collaboration, :, H. Abdalla +234

Dwarf spheroidal galaxies are among the most promising targets for detecting signals of Dark Matter (DM) annihilations. The H.E.S.S. experiment has observed five of these systems f…

astro-ph.HE2018★ 44 cited

First Ground-based Measurement of Sub-20 GeV to 100 GeV -rays from the Vela Pulsar with H.E.S.S. II

H. E. S. S. Collaboration, H. Abdalla, F. Aharonian +230

We report on the measurement and investigation of pulsed high-energy -ray emission from the Vela pulsar, PSR B083345, based on 40.3 hours of observations with the largest tel…

astro-ph.HE2018★ 50 cited

The -ray spectrum of the core of Centaurus A as observed with H.E.S.S. and Fermi-LAT

H. E. S. S. Collaboration, H. Abdalla, A. Abramowski +249

Centaurus A (Cen A) is the nearest radio galaxy discovered as a very-high-energy (VHE; 100 GeV-100 TeV) -ray source by the High Energy Stereoscopic System (H.E.S.S.). It is a fa…

astro-ph.HE2018★ 36 cited

Magnetic Mirroring and Focusing of Cosmic Rays

Kedron Silsbee, Alexei V. Ivlev, Marco Padovani +1

We study the combined impact of magnetic mirroring and focusing on the ionization by cosmic rays (CRs) in dense molecular clouds and circumstellar disks. We show that for effective…

astro-ph.HE2018★ 61 cited

The starburst galaxy NGC 253 revisited by H.E.S.S. and Fermi-LAT

H. E. S. S. Collaboration, H. Abdalla, F. Aharonian +231

(Abridged) Context. NGC 253 is one of only two starburst galaxies found to emit -rays from hundreds of MeV to multi-TeV energies. Accurate measurements of the very-high-energy (…

astro-ph.HE2018★ 186 cited

Cosmic-ray ionisation in circumstellar discs

Marco Padovani, Alexei V. Ivlev, Daniele Galli +1

Galactic cosmic rays are a ubiquitous source of ionisation of the interstellar gas, competing with UV and X-ray photons as well as natural radioactivity in determining the fraction…

astro-ph.HE2018★ 33 cited

H.E.S.S. discovery of very high energy gamma-ray emission from PKS 0625-354

H. E. S. S. Collaboration, H. Abdalla, A. Abramowski +253

PKS 0625-354 (z=0.055) was observed with the four H.E.S.S. telescopes in 2012 during 5.5 hours. The source was detected above an energy threshold of 200 GeV at a significance level…

astro-ph.HE2018★ 69 cited

Population study of Galactic supernova remnants at very high -ray energies with H.E.S.S.

H. E. S. S. Collaboration, :, H. Abdalla +252

Shell-type supernova remnants (SNRs) are considered prime candidates for the acceleration of Galactic cosmic rays (CRs) up to the knee of the CR spectrum at $\mathrm{E} \approx \ma…

astro-ph.HE2018★ 14 cited

Detection of variable VHE gamma-ray emission from the extra-galactic gamma-ray binary LMC P3

H. E. S. S. Collaboration, H. Abdalla, A. Abramowski +253

Context. Recently, the high-energy (HE, 0.1-100 GeV) -ray emission from the object LMC P3 in the Large Magellanic Cloud (LMC) has been discovered to be modulated with a 10.3-day…

astro-ph.HE2018★ 49 cited

A search for new supernova remnant shells in the Galactic plane with H.E.S.S

H. E. S. S. Collaboration, :, H. Abdalla +263

A search for new supernova remnants (SNRs) has been conducted using TeV gamma-ray data from the H.E.S.S. Galactic plane survey. As an identification criterion, shell morphologies t…

astro-ph.HE2017★ 64 cited

TeV gamma-ray observations of the binary neutron star merger GW170817 with H.E.S.S

H. E. S. S. Collaboration, :, H. Abdalla +250

We search for high-energy gamma-ray emission from the binary neutron star merger GW170817 with the H.E.S.S. Imaging Air Cherenkov Telescopes. The observations presented here have b…

astro-ph.HE2017★ 10 cited

Contributions of the High Energy Stereoscopic System (H.E.S.S.) to the 35th International Cosmic Ray Conference (ICRC), Busan, Korea

H. E. S. S. Collaboration, :, H. Abdalla +256

Index of H.E.S.S. conference proceedings to the 35th ICRC, Busan, Korea

astro-ph.HE2017★ 74 cited

Characterising the VHE diffuse emission in the central 200 parsecs of our Galaxy with H.E.S.S

H. E. S. S. Collaboration, :, H. Abdalla +256

The diffuse very high-energy (VHE, > 100 GeV) gamma-ray emission observed in the central 200 pc of the Milky Way by H.E.S.S. was found to follow the dense matter distribution in th…

astro-ph.HE2017★ 82 cited

A polarized fast radio burst at low Galactic latitude

E. Petroff, S. Burke-Spolaor, E. F. Keane +35

We report on the discovery of a new fast radio burst, FRB 150215, with the Parkes radio telescope on 2015 February 15. The burst was detected in real time with a dispersion measure…

astro-ph.HE2017★ 18 cited

Systematic search for very-high-energy gamma-ray emission from bow shocks of runaway stars

H. E. S. S. Collaboration, :, H. Abdalla +260

Runaway stars form bow shocks by ploughing through the interstellar medium at supersonic speeds and are promising sources of non-thermal emission of photons. One of these objects h…