The evolution and structure of pulsar wind nebulae
BM Gaensler, PO Slane - Annu. Rev. Astron. Astrophys., 2006 - annualreviews.org
Pulsars steadily dissipate their rotational energy via relativistic winds. Confinement of these
outflows generates luminous pulsar wind nebulae, seen across the electromagnetic …
outflows generates luminous pulsar wind nebulae, seen across the electromagnetic …
Supernova remnants and γ-ray sources
A review of the possible relationship between γ-ray sources and supernova remnants
(SNRs) is presented. Particular emphasis is given to the analysis of the observational status …
(SNRs) is presented. Particular emphasis is given to the analysis of the observational status …
Pulsar wind nebulae in evolved supernova remnants
JM Blondin, RA Chevalier… - The Astrophysical …, 2001 - iopscience.iop.org
For pulsars similar to the one in the Crab Nebula, most of the energy input to the
surrounding wind nebula occurs on a timescale≲ 10 3 yr; during this time, the nebula …
surrounding wind nebula occurs on a timescale≲ 10 3 yr; during this time, the nebula …
Low-latency gravitational-wave alerts for multimessenger astronomy during the second Advanced LIGO and virgo observing run
BP Abbott, R Abbott, TD Abbott… - The Astrophysical …, 2019 - iopscience.iop.org
Gravitational-wave (GW) multimessenger astronomy provides a unique view of the cosmos.
In this paper, we explain the procedures used during the second observing run of the …
In this paper, we explain the procedures used during the second observing run of the …
Milagro observations of multi-TeV emission from Galactic sources in the Fermi bright source list
We present the result of a search of the Milagro sky map for spatial correlations with sources
from a subset of the recent Fermi Bright Source List (BSL). The BSL consists of the 205 most …
from a subset of the recent Fermi Bright Source List (BSL). The BSL consists of the 205 most …
Observation of supernova remnant IC 443 with the Fermi large area telescope
We report observation of the supernova remnant (SNR) IC 443 (G189. 1+ 3.0) with the Fermi
Gamma-ray Space Telescope Large Area Telescope (LAT) in the energy band between 200 …
Gamma-ray Space Telescope Large Area Telescope (LAT) in the energy band between 200 …
Searches for continuous gravitational waves from 15 supernova remnants and Fomalhaut b with advanced LIGO
BP Abbott, R Abbott, TD Abbott… - The Astrophysical …, 2019 - iopscience.iop.org
With the detections of several binary black hole mergers (Abbott et al. 2016b, 2016c, 2017e,
2017f, 2017g) and one binary neutron star merger (Abbott et al. 2017h) also seen in …
2017f, 2017g) and one binary neutron star merger (Abbott et al. 2017h) also seen in …
Discovery of very high energy gamma radiation from IC 443 with the MAGIC telescope
J Albert, E Aliu, H Anderhub, P Antoranz… - The Astrophysical …, 2007 - iopscience.iop.org
We report the detection of a new source of very high energy (VHE; E γ≥ 100 GeV) γ-ray
emission located close to the Galactic plane, MAGIC J0616+ 225, which is spatially …
emission located close to the Galactic plane, MAGIC J0616+ 225, which is spatially …
Chandra imaging of the X-Ray nebula powered by pulsar B1509–58
BM Gaensler, J Arons, VM Kaspi… - The Astrophysical …, 2002 - iopscience.iop.org
We present observations with the Chandra X-Ray Observatory of the pulsar wind nebula
(PWN) powered by the energetic young pulsar B1509-58. These data confirm the …
(PWN) powered by the energetic young pulsar B1509-58. These data confirm the …
Observation of extended very high energy emission from the supernova remnant IC 443 with VERITAS
VA Acciari, E Aliu, T Arlen, T Aune… - The Astrophysical …, 2009 - iopscience.iop.org
We present evidence that the very high energy (VHE, E> 100 GeV) gamma-ray emission
coincident with the supernova remnant IC 443 is extended. IC 443 contains one of the best …
coincident with the supernova remnant IC 443 is extended. IC 443 contains one of the best …