BeppoSAX observation of the composite remnant G327.1–1.1
Author:
Publisher
EDP Sciences
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://www.aanda.org/10.1051/0004-6361:20021650/pdf
Reference20 articles.
1. Abundances of the elements: Meteoritic and solar
2. BeppoSAX, the wide band mission for X-ray astronomy
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4. Modeling W44 as a Supernova Remnant in a Density Gradient with a Partially Formed Dense Shell and Thermal Conduction in the Hot Interior. I. The Analytical Model
5. The high energy instrument PDS on-board the BeppoSAX X–ray astronomy satellite
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1. MeV–GeV Gamma-Ray Emission from SNR G327.1–1.1 Discovered by the Fermi-LAT;The Astrophysical Journal;2022-11-30
2. Likely Detection of GeV Gamma-Ray Emission from the Composite Supernova Remnant COMP G327.1+1.1 with Fermi-LAT;The Astrophysical Journal;2021-05-01
3. The gas-to-extinction ratio and the gas distribution in the Galaxy;Monthly Notices of the Royal Astronomical Society;2017-06-23
4. RADIO POLARIZATION OBSERVATIONS OF THE SNAIL: A CRUSHED PULSAR WIND NEBULA IN G327.1–1.1 WITH A HIGHLY ORDERED MAGNETIC FIELD;The Astrophysical Journal;2016-03-24
5. LATE-TIME EVOLUTION OF COMPOSITE SUPERNOVA REMNANTS: DEEPCHANDRAOBSERVATIONS AND HYDRODYNAMICAL MODELING OF A CRUSHED PULSAR WIND NEBULA IN SNR G327.1-1.1;The Astrophysical Journal;2015-07-23
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