Pulsar Nebulae-Reference-Cited by-同舟云学术

Pulsar Nebulae

Published:1998 Issue: Volume:188 Page:267-268
ISSN:0074-1809
Container-title:Symposium - International Astronomical Union
language:en
Short-container-title:Symp. - Int. Astron. Union

Author:

Shibata Shinpei,Kawai Nobuyuki,Tamura Keisuke

Abstract

Recent observation with ASCA reveals that radio pulsars own X-ray diffuse nebulae around them. 11 such nebulae have been reported (Harrus, Hughes & Helfand 1996, Shibata et al. 1997, Kawai, Tamura & Shibata 1997). It is most likely that these nebulae are synchrotron nebuale powered by the pulsar wind, the outflow of relativistic particles. Kawai, Tamura and Shibata (1997) reduced an empirical law for the nebula luminosity Lx as a function of the rotation power Ėrot of the central pulsar: Lx/Ėrot = −12.3 + 0.27 log Ėrot.

Publisher

Cambridge University Press (CUP)

Reference7 articles.

1. Shibata S. , Kawai N. , Tamura K. , 1997, submitted to ApJ

2. Discovery of an X-Ray Synchrotron Nebula Associated with the Radio Pulsar PSR B1853+01 in the Supernova Remnant W44

3. X‐Ray Nebula around the Gamma‐Ray Pulsar PSR 1055−52

4. Confinement of the Crab pulsar's wind by its supernova remnant

5. WFPC2 Studies of the Crab Nebula. I. HST and ROSAT Imaging of the Synchrotron Nebula

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