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@article{1804900, author = {Leto, P. and Trigilio, C. and Krtička, Jiří and Fossati, L. and Ignace, R. and Shultz, M. E. and Buemi, C. S. and Cerrigone, L. and Umana, G. and Ingallinera, A. and Bordiu, C. and Pillitteri, I. and Bufano, F. and Oskinova, L. M. and Agliozzo, C. and Cavallaro, F. and Riggi, S. and Loru, S. and Todt, H. and Giarrusso, M. and Phillips, N. M. and Robrade, J. and Leone, F.}, article_number = {2}, doi = {http://dx.doi.org/10.1093/mnras/stab2168}, keywords = {magnetic reconnection; planets and satellites: magnetic fields; stars: early-type; stars: late-type; stars: magnetic field; radio continuum: stars}, language = {eng}, issn = {0035-8711}, journal = {Monthly Notices of the Royal Astronomical Society}, title = {A scaling relationship for non-thermal radio emission from ordered magnetospheres: from the top of the main sequence to planets}, url = {https://academic.oup.com/mnras/article/507/2/1979/6329691}, volume = {507}, year = {2021} }
TY - JOUR ID - 1804900 AU - Leto, P. - Trigilio, C. - Krtička, Jiří - 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. PY - 2021 TI - A scaling relationship for non-thermal radio emission from ordered magnetospheres: from the top of the main sequence to planets JF - Monthly Notices of the Royal Astronomical Society VL - 507 IS - 2 SP - 1979-1998 EP - 1979-1998 PB - Oxford University Press SN - 00358711 KW - magnetic reconnection KW - planets and satellites: magnetic fields KW - stars: early-type KW - stars: late-type KW - stars: magnetic field KW - radio continuum: stars UR - https://academic.oup.com/mnras/article/507/2/1979/6329691 N2 - 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 properties, these stars display a commonality in their radio emission which presents new challenges to the wind scenario as originally conceived. It was thought that relativistic electrons, responsible for the radio emission, originate in current sheets formed, where the wind opens the magnetic field lines. However, the true mass-loss rates from the cooler stars are too small to explain the observed non-thermal broad-band radio spectra. Instead, we suggest the existence of a radiation belt located inside the inner magnetosphere, similar to that of Jupiter. Such a structure explains the overall indifference of the broad-band radio emissions on wind mass-loss rates. Further, correlating the radio luminosities from a larger sample of magnetic stars with their stellar parameters, the combined roles of rotation and magnetic properties have been empirically determined. Finally, our sample of early-type magnetic stars suggests a scaling relationship between the non-thermal radio luminosity and the electric voltage induced by the magnetosphere’s co-rotation, which appears to hold for a broader range of stellar types with dipole-dominated magnetospheres (like the cases of the planet Jupiter and the ultracool dwarf stars and brown dwarfs). We conclude that well-ordered and stable rotating magnetospheres share a common physical mechanism for supporting the generation of non-thermal electrons. ER -
LETO, P., C. TRIGILIO, Jiří KRTIČKA, L. FOSSATI, R. IGNACE, M. E. SHULTZ, C. S. BUEMI, L. CERRIGONE, G. UMANA, A. INGALLINERA, C. BORDIU, I. PILLITTERI, F. BUFANO, L. M. OSKINOVA, C. AGLIOZZO, F. CAVALLARO, S. RIGGI, S. LORU, H. TODT, M. GIARRUSSO, N. M. PHILLIPS, J. ROBRADE a F. LEONE. A scaling relationship for non-thermal radio emission from ordered magnetospheres: from the top of the main sequence to planets. \textit{Monthly Notices of the Royal Astronomical Society}. Oxford University Press, roč.~507, č.~2, s.~1979-1998. ISSN~0035-8711. doi:10.1093/mnras/stab2168. 2021.
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