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Cited article:

BeppoSAX observation of the composite remnant G327.1–1.1

F. Bocchino, R. Bandiera

A&A, 398 1 (2003) 195-202

Published online: 2003-01-14

DOI: https://doi.org/10.1051/0004-6361:20021650

This article has been cited by the following article(s):

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Shock–cloud interactions in the Vela SNR: preliminary results of an XMM-Newton observation

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RADIO POLARIZATION OBSERVATIONS OF THE SNAIL: A CRUSHED PULSAR WIND NEBULA IN G327.1–1.1 WITH A HIGHLY ORDERED MAGNETIC FIELD

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XMM-NewtonandChandraobservations of G272.2-3.2. Evidence of stellar ejecta in the central region

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On the metal abundances inside mixed-morphology supernova remnants: the case of IC 443 and G166.0+4.3

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Enhanced Abundances in Three Large‐Diameter Mixed‐Morphology Supernova Remnants

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Observational data on Galactic supernova remnants III: The supernova remnants within l = 270°-360°

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CHANDRAANDXMMOBSERVATIONS OF THE COMPOSITE SUPERNOVA REMNANT G327.1-1.1

Tea Temim, Patrick Slane, B. M. Gaensler, John P. Hughes and Eric Van Der Swaluw
The Astrophysical Journal 691 (2) 895 (2009)
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Multi-phase interstellar clouds in the Vela SNR resolved with XMM-Newton

M. Miceli, F. Bocchino, A. Maggio and F. Reale
Advances in Space Research 35 (6) 1012 (2005)
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Shock-cloud interaction in the Vela SNR observed with XMM-Newton

M. Miceli, F. Bocchino, A. Maggio and F. Reale
Astronomy & Astrophysics 442 (2) 513 (2005)
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XMM-NewtonandSUZAKUdetection of an X-ray emitting shell around the pulsar wind nebula G54.1+0.3

F. Bocchino, R. Bandiera and J. Gelfand
Astronomy and Astrophysics 520 A71 (2010)
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