activity
20062013
most citedDetection of the Characteristic Pion-Decay Signature in Supernova Remnants

840 citations · 1.2k across the 5 of their papers we have counts for

collaborators

5 papers

astro-ph.HE2013840 cited

Detection of the Characteristic Pion-Decay Signature in Supernova Remnants

LAT collaboration, M. Ackermann, M. Ajello +167

Cosmic rays are particles (mostly protons) accelerated to relativistic speeds. Despite wide agreement that supernova remnants (SNRs) are the sources of galactic cosmic rays, unequi…

astro-ph.HE20131 cited

Probing The Central Engines Of Low-Luminosity Active Galactic Nuclei

Rodrigo Nemmen

I give a brief review of the observational properties of low-luminosity AGNs (LLAGNs). I outline some unresolved issues in the study of LLAGNs, emphasizing the uncertainties in the…

astro-ph.HE2013244 cited

A Universal Scaling for the Energetics of Relativistic Jets From Black Hole Systems

Rodrigo S. Nemmen, Markos Georganopoulos, Sylvain Guiriec +3

Black holes generate collimated, relativistic jets which have been observed in gamma-ray bursts (GRBs), microquasars, and at the center of some galaxies (active galactic nuclei; AG…

astro-ph.HE2012115 cited

Binary Millisecond Pulsar Discovery via Gamma-Ray Pulsations

H. J. Pletsch, L. Guillemot, H. Fehrmann +150

Millisecond pulsars, old neutron stars spun-up by accreting matter from a companion star, can reach high rotation rates of hundreds of revolutions per second. Until now, all such "…

astro-ph2006

Modelling the jet power in elliptical galaxies: support for rapidly spinning black holes

Rodrigo S. Nemmen, Richard G. Bower, Arif Babul +1

Recently, Allen et al. measured a tight correlation between the Bondi accretion rates and jet powers of the nuclei of nearby X-ray luminous elliptical galaxies. We employ two model…