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Просмотр по автору "Loru S."

Просмотр по автору "Loru S."

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  • A scaling relationship for non-thermal radio emission from ordered magnetospheres: From the top of the main sequence to planets 
    Leto P.; Trigilio C.; Krtička J.; Fossati L.; Ignace R.; Shultz M.E.; Buemi C.S.; Cerrigone L.; Umana G.; Ingallinera A.; Bordiu C.; Pillitteri I.; Bufano F.; Oskinova L.M.; Agliozzo C.; Cavallaro F.; Riggi S.; Loru S.; Todt H.; Giarrusso M.; Phillips N.M.; Robrade J.; Leone F. (2021)
    In this paper, we present the analysis of incoherent non-thermal radio emission from a sample of hot magnetic stars, ranging from early-B to early-A spectral type. Spanning a wide range of stellar parameters and wind ...
  • Evidence for radio and x-ray auroral emissions from the magnetic b-type star ρ oph a 
    Leto P.; Trigilio C.; Leone F.; Pillitteri I.; Buemi C.S.; Fossati L.; Cavallaro F.; Oskinova L.M.; Ignace R.; Krtička J.; Umana G.; Catanzaro G.; Ingallinera A.; Bufano F.; Agliozzo C.; Phillips N.M.; Cerrigone L.; Riggi S.; Loru S.; Munari M.; Gangi M.; Giarrusso M.; Robrade J. (2020)
    © 2020 The Author(s) Published by Oxford University Press on behalf of the Royal Astronomical Society We present new ATCA multiwavelength radio measurements (range 2.1–21.2 GHz) of the early-type magnetic star ρ Oph A, ...
  • Investigating the Mini and Giant Radio Flare Episodes of Cygnus X-3 
    Egron E.; Pellizzoni A.; Righini S.; Giroletti M.; Koljonen K.; Pottschmidt K.; Trushkin S.; Lobina J.; Pilia M.; Wilms J.; Corbel S.; Grinberg V.; Loru S.; Trois A.; Rodriguez J.; Lähteenmäki A.; Tornikoski M.; Enestam S.; Järvelä E. (2020)
    © 2020. The American Astronomical Society. All rights reserved. The microquasar Cygnus X-3 underwent a giant radio flare in 2017 April, reaching a maximum flux of ∼16.5 Jy at 8.5 GHz. We present results from a long monitoring ...
  • The auroral radio emission of the magnetic B-type star ρ OphC 
    Leto P.; Trigilio C.; Buemi C.S.; Leone F.; Pillitteri I.; Fossati L.; Cavallaro F.; Oskinova L.M.; Ignace R.; Krtička J.; Umana G.; Catanzaro G.; Ingallinera A.; Bufano F.; Riggi S.; Cerrigone L.; Loru S.; Schilliró F.; Agliozzo C.; Phillips N.M.; Giarrusso M.; Robrade J. (2020)
    © 2020 The Author(s) Published by Oxford University Press on behalf of the Royal Astronomical Society. The non-thermal radio emission of main-sequence early-type stars is a signature of stellar magnetism. We present ...

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