Synthetic X-ray and radio maps for two different models of Stephan's Quintet
Author:
Affiliation:
1. Department of Physics; University of Konstanz; Universitätsstr. 10; 78457; Konstanz; Germany
2. University Observatory Munich; Scheinerstr. 1; 81679; Munich; Germany
Publisher
Oxford University Press (OUP)
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://academic.oup.com/mnras/article-pdf/426/4/3160/3324067/426-4-3160.pdf
Reference58 articles.
1. Radio Continuum Emission at 21 cm near Stephan's Quintet
2. Powerful High-Velocity Dispersion Molecular Hydrogen Associated with an Intergalactic Shock Wave in Stephan's Quintet
3. Neighborhoods of spiral galaxies. I. Multiple interacting galaxies.
4. Magnetic Fields in Galaxies
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2. A Large-scale, Regular Intergalactic Magnetic Field Associated with Stephan’s Quintet?;The Astrophysical Journal;2020-07-29
3. On the origin of magnetic driven winds and the structure of the galactic dynamo in isolated galaxies;Monthly Notices of the Royal Astronomical Society;2020-03-27
4. Redshift effect implications on revised models of Stephan’s Quintet;Modern Physics Letters A;2019-09-17
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