Radio emission from shell-type supernova remnants-Reference-Cited by-同舟云学术

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Radio emission from shell-type supernova remnants

Published:2006-09-12 Issue:2 Volume:459 Page:519-533
ISSN:0004-6361
Container-title:Astronomy & Astrophysics
language:
Short-container-title:A&A

Author:

Asvarov A. I.

Publisher

EDP Sciences

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://www.aanda.org/10.1051/0004-6361:20041155/pdf

Reference70 articles.

1. Asvarov, A. I. 2001, Proc. Symp., 205 IAU, ed. T. Schilizzi, S. Vogel, F. Paresce, & M. Elvis, 398

2. Ballet, J. 2005, Adv. Sp. Res., in press [arXiv:astro-ph/0503309]

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1. SRG/eROSITA discovery of a radio-faint X-ray candidate supernova remnant SRGe J003602.3+605421 = G121.1−1.9;Monthly Notices of the Royal Astronomical Society;2023-03-20

2. Radio Nebulae from Hyperaccreting X-Ray Binaries as Common-envelope Precursors and Persistent Counterparts of Fast Radio Bursts;The Astrophysical Journal;2022-09-01

3. LOFAR detection of faint radio emission from the supernova remnant SRGe J0023+3625 = G116.6−26.1: probing the Milky Way synchrotron halo;Monthly Notices of the Royal Astronomical Society: Letters;2022-04-13

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5. A New, Deep JVLA Radio Survey of M33;The Astrophysical Journal Supplement Series;2019-04-16

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