Constraining the nature of DG Tau A’s thermal and non-thermal radio emission-Reference-Cited by-同舟云学术

Constraining the nature of DG Tau A’s thermal and non-thermal radio emission

Published:2018-10-03 Issue:4 Volume:481 Page:5532-5542
ISSN:0035-8711
Container-title:Monthly Notices of the Royal Astronomical Society
language:en
Short-container-title:

Author:

Purser S J D¹^ORCID,Ainsworth R E¹²^ORCID,Ray T P¹,Green D A³,Taylor A M¹⁴,Scaife A M M²

Affiliation:

1. School of Cosmic Physics, Dublin Institute for Advanced Studies, 31 Fitzwilliam Place, Dublin 2, Ireland

2. Jodrell Bank Centre for Astrophysics, Alan Turing Building, School of Physics and Astronomy, University of Manchester, Oxford Road, Manchester M13 9PL, UK

3. Astrophysics Group, Cavendish Laboratory, 19 J. J. Thomson Avenue, Cambridge CB3 0HE, UK

4. DESY, Platanenallee 6, D-15738 Zeuthen, Germany

Funder

European Research Council

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://academic.oup.com/mnras/article-pdf/481/4/5532/27017321/sty2649.pdf

Reference45 articles.

1. Subarcsecond high-sensitivity measurements of the DG Tau jet with e-MERLIN

2. TENTATIVE EVIDENCE FOR RELATIVISTIC ELECTRONS GENERATED BY THE JET OF THE YOUNG SUN-LIKE STAR DG Tau

3. GMRT detections of low-mass young stars at 323 and 608 MHz

4. Keck Interferometer Observations of Classical and Weak‐line T Tauri Stars

5. AMI-LA radio continuum observations of Spitzer c2d small clouds and cores: Perseus region★

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