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A scaling relationship for nonthermal radio emission from ordered magnetospheres: II. Investigating the efficiency of relativistic electron production in the magnetospheres of BA-type stars

  • P. Leto
  • , S. Owocki
  • , C. Trigilio
  • , F. Cavallaro
  • , B. Das
  • , M. E. Shultz
  • , C. S. Buemi
  • , G. Umana
  • , L. Fossati
  • , R. Ignace
  • , J. Krtička
  • , L. M. Oskinova
  • , I. Pillitteri
  • , C. Bordiu
  • , F. Bufano
  • , L. Cerrigone
  • , A. Ingallinera
  • , S. Loru
  • , S. Riggi
  • , A. C. Ruggeri
  • A. Ud-Doula, F. Leone
  • INAF – Osservatorio Astrofisico di Catania
  • University of Delaware
  • Space and Astronomy
  • Astronomical Research in the Southern Hemisphere
  • Austrian Academy of Sciences
  • Masaryk University
  • Universität Potsdam
  • INAF – Osservatorio Astronomico di Palermo
  • National Radio Astronomy Observatory
  • Joint ALMA Observatory
  • Penn State Scranton
  • Universitá di Catania

Research output: Contribution to journalArticlepeer-review

Original languageEnglish
Article numberA241
JournalAstronomy and Astrophysics
Volume706
DOIs
StatePublished - Feb 1 2026

ASJC Scopus Subject Areas

  • Astronomy and Astrophysics
  • Space and Planetary Science

Keywords

  • Acceleration of particles
  • Magnetic reconnection
  • Radiation mechanisms: non-thermal
  • Radio continuum: stars
  • Stars: early-type
  • Stars: magnetic field

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