LATE-TIME EVOLUTION OF COMPOSITE SUPERNOVA REMNANTS: DEEPCHANDRAOBSERVATIONS AND HYDRODYNAMICAL MODELING OF A CRUSHED PULSAR WIND NEBULA IN SNR G327.1-1.1-Reference-Cited by-同舟云学术

LATE-TIME EVOLUTION OF COMPOSITE SUPERNOVA REMNANTS: DEEPCHANDRAOBSERVATIONS AND HYDRODYNAMICAL MODELING OF A CRUSHED PULSAR WIND NEBULA IN SNR G327.1-1.1

Published:2015-07-23 Issue:1 Volume:808 Page:100
ISSN:1538-4357
Container-title:The Astrophysical Journal
language:
Short-container-title:ApJ

Author:

Temim Tea^ORCID,Slane Patrick^ORCID,Kolb Christopher,Blondin John^ORCID,Hughes John P.,Bucciantini Niccoló

Publisher

American Astronomical Society

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://stacks.iop.org/0004-637X/808/i=1/a=100/pdf

Reference27 articles.

1. FERMILARGE AREA TELESCOPE OBSERVATIONS OF THE VELA-X PULSAR WIND NEBULA

2. CONSTRAINTS ON THE GALACTIC POPULATION OF TeV PULSAR WIND NEBULAE USINGFERMILARGE AREA TELESCOPE OBSERVATIONS

3. Abundances of the elements: Meteoritic and solar

4. Pulsar Wind Nebulae in Evolved Supernova Remnants

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