Tracing star formation with non-thermal radio emission-Reference-Cited by-同舟云学术

Tracing star formation with non-thermal radio emission

Published:2017-02-22 Issue:1 Volume:468 Page:946-958
ISSN:0035-8711
Container-title:Monthly Notices of the Royal Astronomical Society
language:en
Short-container-title:

Author:

Schober Jennifer¹,Schleicher D. R. G.²,Klessen R. S.³⁴

Affiliation:

1. Nordita, KTH Royal Institute of Technology and Stockholm University, Roslagstullsbacken 23, SE-10691 Stockholm, Sweden

2. Departamento de Astronomía, Facultad Ciencias Físicas y Matemáticas, Universidad de Concepción, Av. Esteban Iturra s/n Barrio Universitario, Casilla 160-C, Concepción, Chile

3. Universität Heidelberg, Zentrum für Astronomie, Institut für Theoretische Astrophysik, Albert-Ueberle-Strasse 2, D-69120 Heidelberg, Germany

4. Universität Heidelberg, Interdisziplinäres Zentrum für Wissenschaftliches Rechnen, Im Neuenheimer Feld 205, D-69120 Heidelberg, Germany

Funder

CATA

ERC

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://academic.oup.com/mnras/article-pdf/468/1/946/11114341/stx460.pdf

Reference100 articles.

1. M 82 – A radio continuum and polarisation study

2. Starburst in the Ultraluminous Galaxy Arp 220: Constraints from Observations of Radio Recombination Lines and Continuum

3. The Far‐ and Mid‐Infrared/Radio Correlations in the Spitzer Extragalactic First Look Survey

4. Magnetism in the spiral galaxy NGC 6946: magnetic arms, depolarization rings, dynamo modes, and helical fields

5. Magnetic fields in spiral galaxies

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