An Analysis of the Broadband (22-3900 MHz) Radio Spectrum of HB 3 (G132.7+1.3): The Detection of Thermal Radio Emission from an Evolved Supernova Remnant?-Reference-Cited by-同舟云学术

An Analysis of the Broadband (22-3900 MHz) Radio Spectrum of HB 3 (G132.7+1.3): The Detection of Thermal Radio Emission from an Evolved Supernova Remnant?

Published:2007-01-10 Issue:1 Volume:655 Page:L41-L44
ISSN:0004-637X
Container-title:The Astrophysical Journal
language:en
Short-container-title:ApJ

Author:

Urošević D.,Pannuti T. G.,Leahy D.

Publisher

American Astronomical Society

Subject

Space and Planetary Science,Astronomy and Astrophysics

Reference15 articles.

1. Blackburn, J. K. 1995, in ASP Conf. Ser. 77, Astronomical Data Analysis Software and Systems IV, ed. R. A. Shaw, H. E. Payne, & J. J. E. Hayes (San Francisco: ASP), 367

2. A Survey of 23 Localized Radio Sources in the Northern Hemisphere

3. Green, D. A. 2006, A Catalogue of Galactic Supernova Remnants, 2006 April Ver. (Cambridge: Astrophysics Group, Cavendish Laboratory, Univ. Cambridge), http://www.mrao.cam.ac.uk/surveys/snrs/

4. Shock-excited Maser Emission from Supernova Remnants: G32.8−0.1, G337.8−0.1, G346.6−0.2, and the HB 3/W3 Complex

5. Observations at 408 MHz of the supernova remnant HB 3 (G132.6 + 1.5)

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