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29 papers · 1 filter
ASTRO-H White Paper - New Spectral Features
R. K. Smith, H. Odaka, M. Audard +27
This white paper addresses selected new (to X-ray astronomy) physics and data analysis issues that will impact ASTRO-H SWG observations as a result of its high-spectral-resolution…
ASTRO-H White Paper - Young Supernova Remnants
J. P. Hughes, S. Safi-Harb, A. Bamba +23
Thanks to the unprecedented spectral resolution and sensitivity of the Soft X-ray Spectrometer (SXS) to soft thermal X-ray emission, ASTRO-H will open a new discovery window for un…
ASTRO-H White Paper - Older Supernova Remnants and Pulsar Wind Nebulae
K. S. Long, A. Bamba, F. Aharonian +20
Most supernova remnants (SNRs) are old, in the sense that their structure has been profoundly modified by their interaction with the surrounding interstellar medium (ISM). Old SNRs…
Unprecedented study of the broadband emission of Mrk 421 during flaring activity in March 2010
The MAGIC Collaboration, J. Aleksić, S. Ansoldi +251
A flare from the TeV blazar Mrk 421, occurring in March 2010, was observed for 13 consecutive days from radio to very high energy (VHE, E > 100 GeV) gamma-rays with MAGIC, VERITAS,…
On cosmic-ray production efficiency at supernova remnant shocks propagating into realistic diffuse interstellar medium
Jiro Shimoda, Tsuyoshi Inoue, Yutaka Ohira +3
Using three-dimensional magnetohydrodynamics simulations, we show that the efficiency of cosmic-ray (CR) production at supernova remnants (SNRs) is over-predicted if it could be es…
Broken time-reversal symmetry probed by muon spin relaxation in the caged type superconductor LuRhSn
A. Bhattacharyya, D. T. Adroja, J. Quintanilla +4
The superconducting state of the caged type compound LuRhSn has been investigated by using magnetization, heat capacity, and muon-spin relaxation or rotation (SR)…