Results 11 to 20 of about 8,336 (234)
The imprint of pulsar parameters on the morphology of Pulsar Wind Nebulae [PDF]
Monthly Notices of the Royal Astronomical Society, 2016 The morphology of young Pulsar Wind Nebulae (PWN) is largely determined by the properties of the wind injected by the pulsar. We have used a recent parametrization of the wind obtained from Force Free Electrodynamics simulations of pulsar magnetospheres ...
Buehler, Rolf, Giomi, Matteo
core +4 more sources
Pulsar wind nebulae in supernova remnants [PDF]
Astronomy and Astrophysics, 2000 A spherically symmetric model is presented for the interaction of a pulsar wind with the associated supernova remnant. This results in a pulsar wind nebula whose evolution is coupled to the evolution of the surrounding supernova remnant.
Achterberg, A. +3 more
core +4 more sources
The Pulsar Wind Nebula of the Geminga Pulsar [PDF]
The Astrophysical Journal, 2006 Revised version: data analysis described in more detail, Figure 2 replaced; 6 pages, 2 color figures; accepted for publication in ApJ (v.643, 2006 June 1)
George G. Pavlov +2 more
openalex +4 more sources
The Pulsar Wind Nebula in G11.2−0.3 [PDF]
The Astrophysical Journal, 2003 4 pages, 2 figures, To appear in "Neutron Stars in Supernova Remnants" (ASP Conference Proceedings), eds P. O. Slane and B.
M. S. Roberts +7 more
openalex +6 more sources
Optical identification of the 3C 58 pulsar wind nebula [PDF]
, 2008 We have performed a deep optical imaging of 3C 58 SNR with the NOT in the B and V bands to detect the optical counterpart of the associated pulsar J0295+6449 and its torus-like wind nebula visible in X-rays.
Yu. A. Shibanov +4 more
openalex +5 more sources
The Supernova Remnant G106.3+2.7 and Its Pulsar‐Wind Nebula: Relics of Triggered Star Formation in a Complex Environment [PDF]
, 2001 We propose that the pulsar nebula associated with the pulsar J2229+6114 and the supernova remnant (SNR) G106.3+2.7 are the result of the same supernova explosion.
R. Kothes +2 more
openalex +4 more sources
ChandraConfirmation of a Pulsar Wind Nebula in DA 495 [PDF]
, 2008 As part of a multiwavelength study of the unusual radio supernova remnant DA 495, we present observations made with the Chandra X-ray Observatory. Imaging and spectroscopic analysis confirms the previously detected X-ray source at the heart of the ...
Zaven Arzoumanian +4 more
openalex +3 more sources
MULTI-ZONE MODELING OF THE PULSAR WIND NEBULA HESS J1825–137 [PDF]
, 2011 The pulsar wind nebula associated with PSR J1826-1334, HESS J1825-137, is a bright very high energy source with an angular extent of ~1 degree and spatially-resolved spectroscopic TeV measurements.
A. Van Etten, Roger W. Romani
openalex +3 more sources
Journal of Geophysical Research: Space Physics, Volume 128, Issue 2, February 2023., 2023 Abstract We present long‐term density trends of the Earth's upper atmosphere at altitudes between 71 and 116 km, based on atmospheric occultations of the Crab Nebula observed with X‐ray astronomy satellites, ASCA, RXTE, Suzaku, NuSTAR, and Hitomi. The combination of the five satellites provides a time period of 28 years from 1994 to 2022.
Satoru Katsuda +11 more
wiley +1 more source
A search for runaway stars in 12 Galactic supernova remnants
Astronomische Nachrichten, Volume 342, Issue 3, Page 553-577, March 2021., 2021 Runaway stars can result from core‐collapse supernovae in multiple stellar systems. If the supernova disrupts the system, the companion is ejected with its former orbital velocity. A clear identification of a runaway star can yield the time and place of the explosion, as well as orbital parameters of the pre‐supernova binary system.
Oliver Lux +3 more
wiley +1 more source