The physical parameters of the microquasar S26 in the Sculptor Group galaxy NGC 7793-Reference-Cited by-同舟云学术

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The physical parameters of the microquasar S26 in the Sculptor Group galaxy NGC 7793

Published:2012-11-05 Issue:2 Volume:427 Page:956-967
ISSN:0035-8711
Container-title:Monthly Notices of the Royal Astronomical Society
language:en
Short-container-title:Monthly Notices of the Royal Astronomical Society

Author:

Dopita M. A.,Payne J. L.¹,Filipović M. D.¹,Pannuti T. G.²

Affiliation:

1. University of Western Sydney; School of Computing; Engineering and Mathematics; Locked Bag 1797; Penrith South DC; NSW; 2751; Australia

2. Department of Earth and Space Sciences; Space Science Center; Morehead State University; Morehead; KY; 40351; USA

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://academic.oup.com/mnras/article-pdf/427/2/956/3005443/427-2-956.pdf

Reference38 articles.

1. The MAPPINGS III Library of Fast Radiative Shock Models

2. Unification of the Radio and Optical Properties of Gigahertz Peak Spectrum and Compact Steep‐Spectrum Radio Sources

3. Identification of Supernova Remnants in the Sculptor Group Galaxies NGC 300 and NGC 7793

4. A 'Twin-Exhaust' Model for Double Radio Sources

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4. The supernova remnant populations of the galaxies NGC 45, NGC 55, NGC 1313, NGC 7793: luminosity and excitation functions;Monthly Notices of the Royal Astronomical Society;2021-08-23

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