Radio-continuum study of the nearby sculptor group galaxies. Part 3: NGC 7793 at λ=12.2, 6 and 3 cm
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Published:2014-10
Issue:2
Volume:353
Page:603-611
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ISSN:0004-640X
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Container-title:Astrophysics and Space Science
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language:en
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Short-container-title:Astrophys Space Sci
Author:
Galvin Timothy J.,Filipović Miroslav D.,Tothill Nicholas F. H.,Crawford Evan J.,O’Brien Andrew N.,Seymour Nicholas,Pannuti Thomas G.,Kosakowski Alekzander R.,Sharma Biswas
Publisher
Springer Science and Business Media LLC
Subject
Space and Planetary Science,Astronomy and Astrophysics
Reference18 articles.
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10.1088/0004-637X/703/1/517 3. Dopita, M.A., Payne, J.L., Filipović, M.D., Pannuti, T.G.: The physical parameters of the microquasar S26 in the Sculptor Group galaxy NGC 7793. Mon. Not. R. Astron. Soc. 427, 956–967 (2012). doi:
10.1111/j.1365-2966.2012.21947.x 4. Galvin, T.J., Filipović, M.D., Crawford, E.J., Wong, G., Payne, J.L., De Horta, A., White, G.L., Tothill, N., Drašković, D., Pannuti, T.G., Grimes, C.K., Cahall, B.J., Millar, W.C., Laine, S.: Radio-continuum study of the Nearby sculptor group galaxies. Part 1: NGC 300 at λ=20 cm. Astrophys. Space Sci. 340, 133–142 (2012). doi:
10.1007/s10509-012-1044-3 5. Gooch, R.: Karma: Visualisation Test-Bed Toolkit, February 2011. Astrophysics Source Code Library
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