Results 91 to 100 of about 8,188 (190)

An Unusual Pulsar Wind Nebula Associated with PSR B0906−49 [PDF]

, 1998
B. M. Gaensler, B. W. Stappers, D. A. Frail, S. Johnston   +3 more
openalex   +1 more source

Multiwavelength Observations of Pulsar Wind Nebulae [PDF]

, 2010
20 pages, 11 figures. Invited review to appear in Proc. of the inaugural ICREA Workshop on "The High-Energy Emission from Pulsars and their Systems" (2010), eds. N. Rea and D. Torres, (Springer Astrophysics and Space Science series)
openaire   +3 more sources

High energy processes in pulsar wind nebulae [PDF]

Astrophysics and Space Science, 2007
9 pages, 1 figure, Proc.
openaire   +3 more sources

Variability of the Vela Pulsar Wind Nebula Observed with [ITAL]Chandra[/ITAL] [PDF]

, 2001
George G. Pavlov, Oleg Kargaltsev, D. Sanwal, G. P. Garmire   +3 more
openalex   +1 more source

X‐Ray Thread G0.13−0.11: A Pulsar Wind Nebula? [PDF]

, 2002
Q. Daniel Wang, F. J. Lu, Cornelia Lang
openalex   +1 more source

Discovery of a radio emitting neutron star with an ultra-long spin period of 76 seconds. [PDF]

Nat Astron, 2022
Caleb M, Heywood I, Rajwade K, Malenta M, Stappers B, Barr E, Chen W, Morello V, Sanidas S, van den Eijnden J, Kramer M, Buckley D, Brink J, Motta SE, Woudt P, Weltevrede P, Jankowski F, Surnis M, Buchner S, Bezuidenhout MC, Driessen LN, Fender R.   +21 more
europepmc   +1 more source

Pulsar-wind nebulae in X-rays and TeV gamma-rays

, 2010
Pulsars are known to be efficient accelerators that produce copious amounts of relativistic particles and inject them into the Galactic medium. The radiation emitted by such a pulsar wind can be seen from radio through gamma-rays as a pulsar-wind nebula (
Kargaltsev, Oleg, Pavlov, George
core   +1 more source

Three Concurrent Phases of Massive-Star Evolution in a Pulsar-Wind Nebula [PDF]

, 2010
The nebular material associated the the SNR G54.1+0.3 (hereafter G54) contains the the first reported instance of triggered star formation in the immediate vicinity of a Pulsar and its Wind Nebula (PWN). With 2MASS and Spitzer colors and followup near-IR
Hillier, D. John, Lang, Cornelia, Mauerhan, Jon, Morris, Patrick, Van Dyk, Schuyler   +4 more
core  

The variable Crab Nebula

, 2011
The remarkable Crab Nebula is powered by an energetic pulsar whose relativistic wind interacts with the inner parts of the Supernova Remnant SN1054. Despite low-intensity optical and X-ray variations in the inner Nebula, the Crab has been considered ...
Tavani, Marco
core   +1 more source

A Multifrequency Radio Study of Supernova Remnant G292.0+1.8 and Its Pulsar Wind Nebula [PDF]

, 2003
B. M. Gaensler, B. J. Wallace
openalex   +1 more source