The population of M dwarfs observed at low radio frequencies-Reference-Cited by-同舟云学术

The population of M dwarfs observed at low radio frequencies

Published:2021-10-11 Issue:12 Volume:5 Page:1233-1239
ISSN:2397-3366
Container-title:Nature Astronomy
language:en
Short-container-title:Nat Astron

Author:

Callingham J. R.^ORCID,Vedantham H. K.^ORCID,Shimwell T. W.^ORCID,Pope B. J. S.^ORCID,Davis I. E.,Best P. N.^ORCID,Hardcastle M. J.,Röttgering H. J. A.,Sabater J.^ORCID,Tasse C.,van Weeren R. J.^ORCID,Williams W. L.^ORCID,Zarka P.^ORCID,de Gasperin F.,Drabent A.^ORCID

Publisher

Springer Science and Business Media LLC

Subject

Astronomy and Astrophysics

Link

https://www.nature.com/articles/s41550-021-01483-0.pdf

Reference64 articles.

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3. Zarka, P. Plasma interactions of exoplanets with their parent star and associated radio emissions. Planet. Space Sci. 55, 598–617 (2007).

4. Turnpenney, S., Nichols, J. D., Wynn, G. A. & Burleigh, M. R. Exoplanet-induced radio emission from M dwarfs. Astrophys. J. 854, 72 (2018).

5. Villadsen, J. & Hallinan, G. Ultra-wideband detection of 22 coherent radio bursts on M dwarfs. Astrophys. J. 871, 214 (2019).

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