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A scaling relationship for non-thermal radio emission from ordered magnetospheres: From the top of the main sequence to planets

  • P. Leto
  • , C. Trigilio
  • , J. Krtička
  • , L. Fossati
  • , R. Ignace
  • , M. E. Shultz
  • , C. S. Buemi
  • , L. Cerrigone
  • , G. Umana
  • , A. Ingallinera
  • , C. Bordiu
  • , I. Pillitteri
  • , F. Bufano
  • , Lidia M. Oskinova
  • , C. Agliozzo
  • , F. Cavallaro
  • , S. Riggi
  • , S. Loru
  • , H. Todt
  • , M. Giarrusso
  • N. M. Phillips, J. Robrade, F. Leone
  • INAF – Osservatorio Astrofisico di Catania
  • Masaryk University
  • Austrian Academy of Sciences
  • University of Delaware
  • Joint ALMA Observatory
  • CSIC-INTA - Centro de Astrobiología (CAB)
  • INAF – Osservatorio Astronomico di Palermo
  • Universität Potsdam
  • Kazan Federal University
  • ESO-European Organisation for Astronomical Research in the Southern Hemisphere
  • Inter-University Institute for Data Intensive Astronomy (IDIA)
  • Laboratori Nazionali del Sud
  • University of Hamburg
  • Universitá di Catania

Research output: Contribution to journalArticlepeer-review

Original languageEnglish
Pages (from-to)1979-1998
Number of pages20
JournalMonthly Notices of the Royal Astronomical Society
Volume507
Issue number2
DOIs
StatePublished - Oct 1 2021

ASJC Scopus Subject Areas

  • Astronomy and Astrophysics
  • Space and Planetary Science

Keywords

  • magnetic reconnection
  • planets and satellites: magnetic fields
  • radio continuum: stars
  • stars: early-type
  • stars: late-type
  • stars: magnetic field

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