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

Result code in IS VaVaI

<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F00216224%3A14310%2F21%3A00122951" target="_blank" >RIV/00216224:14310/21:00122951 - isvavai.cz</a>

Result on the web

<a href="https://academic.oup.com/mnras/article/507/2/1979/6329691" target="_blank" >https://academic.oup.com/mnras/article/507/2/1979/6329691</a>

DOI - Digital Object Identifier

<a href="http://dx.doi.org/10.1093/mnras/stab2168" target="_blank" >10.1093/mnras/stab2168</a>

Result language

angličtina

Original language name

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

Original language description

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.

Czech name

—

Czech description

—

Type

J_imp - Article in a specialist periodical, which is included in the Web of Science database

CEP classification

—

OECD FORD branch

10308 - Astronomy (including astrophysics,space science)

Project

—

Continuities

I - Institucionalni podpora na dlouhodoby koncepcni rozvoj vyzkumne organizace

Publication year

2021

Confidentiality

S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů

Name of the periodical

Monthly Notices of the Royal Astronomical Society

ISSN

0035-8711

e-ISSN

1365-2966

Volume of the periodical

507

Issue of the periodical within the volume

2

Country of publishing house

GB - UNITED KINGDOM

Number of pages

20

Pages from-to

1979-1998

UT code for WoS article

000697380800029

EID of the result in the Scopus database

2-s2.0-85115436622