A combined multiwavelength VLA/ALMA/Chandra study unveils the complex magnetosphere of the B-type star HR5907

P. Leto, C. Trigilio, L. M. Oskinova, R. Ignace, C. S. Buemi, G. Umana, A. Ingallinera, F. Leone, N. M. Phillips, C. Agliozzo, H. Todt, L. Cerrigone

Resultado de la investigación: Article

3 Citas (Scopus)

Resumen

We present new radio/millimeter measurements of the hot magnetic star HR5907 obtained with the VLA and ALMA interferometers. We find that HR5907 is the most radio luminous early type star in the cm-mm band among those presently known. Its multi-wavelength radio light curves are strongly variable with an amplitude that increases with radio frequency. The radio emission can be explained by the populations of the non-thermal electrons accelerated in the current sheets on the outer border of the magnetosphere of this fast-rotating magnetic star. We classify HR5907 as another member of the growing class of strongly magnetic fastrotating hot stars where the gyro-synchrotron emission mechanism efficiently operates in their magnetospheres. The new radio observations of HR5907 are combined with archival X-ray data to study the physical condition of its magnetosphere. The X-ray spectra of HR5907 show tentative evidence for the presence of non-thermal spectral component. We suggest that non-thermal X-rays originate a stellar X-ray aurora due to streams of non-thermal electrons impacting on the stellar surface. Taking advantage of the relation between the spectral indices of the X-ray power-law spectrum and the non-thermal electron energy distributions, we perform 3-D modelling of the radio emission for HR5907. The wavelength-dependent radio light curves probe magnetospheric layers at different heights above the stellar surface. A detailed comparison between simulated and observed radio light curves leads us to conclude that the stellar magnetic field of HR 5907 is likely non-dipolar, providing further indirect evidence of the complex magnetic field topology of HR5907.

Idioma originalEnglish
Páginas (desde-hasta)562-579
Número de páginas18
PublicaciónMonthly Notices of the Royal Astronomical Society
Volumen476
N.º1
DOI
EstadoPublished - 1 may 2018

Huella dactilar

magnetospheres
magnetosphere
magnetic stars
radio
stars
light curve
hot stars
radio emission
x rays
stellar magnetic fields
radio observation
current sheets
electron
borders
wavelengths
radio frequencies
energy distribution
synchrotrons
electrons
topology

ASJC Scopus subject areas

  • Astronomy and Astrophysics
  • Space and Planetary Science

Citar esto

Leto, P. ; Trigilio, C. ; Oskinova, L. M. ; Ignace, R. ; Buemi, C. S. ; Umana, G. ; Ingallinera, A. ; Leone, F. ; Phillips, N. M. ; Agliozzo, C. ; Todt, H. ; Cerrigone, L. / A combined multiwavelength VLA/ALMA/Chandra study unveils the complex magnetosphere of the B-type star HR5907. En: Monthly Notices of the Royal Astronomical Society. 2018 ; Vol. 476, N.º 1. pp. 562-579.
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title = "A combined multiwavelength VLA/ALMA/Chandra study unveils the complex magnetosphere of the B-type star HR5907",
abstract = "We present new radio/millimeter measurements of the hot magnetic star HR5907 obtained with the VLA and ALMA interferometers. We find that HR5907 is the most radio luminous early type star in the cm-mm band among those presently known. Its multi-wavelength radio light curves are strongly variable with an amplitude that increases with radio frequency. The radio emission can be explained by the populations of the non-thermal electrons accelerated in the current sheets on the outer border of the magnetosphere of this fast-rotating magnetic star. We classify HR5907 as another member of the growing class of strongly magnetic fastrotating hot stars where the gyro-synchrotron emission mechanism efficiently operates in their magnetospheres. The new radio observations of HR5907 are combined with archival X-ray data to study the physical condition of its magnetosphere. The X-ray spectra of HR5907 show tentative evidence for the presence of non-thermal spectral component. We suggest that non-thermal X-rays originate a stellar X-ray aurora due to streams of non-thermal electrons impacting on the stellar surface. Taking advantage of the relation between the spectral indices of the X-ray power-law spectrum and the non-thermal electron energy distributions, we perform 3-D modelling of the radio emission for HR5907. The wavelength-dependent radio light curves probe magnetospheric layers at different heights above the stellar surface. A detailed comparison between simulated and observed radio light curves leads us to conclude that the stellar magnetic field of HR 5907 is likely non-dipolar, providing further indirect evidence of the complex magnetic field topology of HR5907.",
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author = "P. Leto and C. Trigilio and Oskinova, {L. M.} and R. Ignace and Buemi, {C. S.} and G. Umana and A. Ingallinera and F. Leone and Phillips, {N. M.} and C. Agliozzo and H. Todt and L. Cerrigone",
year = "2018",
month = "5",
day = "1",
doi = "10.1093/mnras/sty244",
language = "English",
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Leto, P, Trigilio, C, Oskinova, LM, Ignace, R, Buemi, CS, Umana, G, Ingallinera, A, Leone, F, Phillips, NM, Agliozzo, C, Todt, H & Cerrigone, L 2018, 'A combined multiwavelength VLA/ALMA/Chandra study unveils the complex magnetosphere of the B-type star HR5907', Monthly Notices of the Royal Astronomical Society, vol. 476, n.º 1, pp. 562-579. https://doi.org/10.1093/mnras/sty244

A combined multiwavelength VLA/ALMA/Chandra study unveils the complex magnetosphere of the B-type star HR5907. / Leto, P.; Trigilio, C.; Oskinova, L. M.; Ignace, R.; Buemi, C. S.; Umana, G.; Ingallinera, A.; Leone, F.; Phillips, N. M.; Agliozzo, C.; Todt, H.; Cerrigone, L.

En: Monthly Notices of the Royal Astronomical Society, Vol. 476, N.º 1, 01.05.2018, p. 562-579.

Resultado de la investigación: Article

TY - JOUR

T1 - A combined multiwavelength VLA/ALMA/Chandra study unveils the complex magnetosphere of the B-type star HR5907

AU - Leto, P.

AU - Trigilio, C.

AU - Oskinova, L. M.

AU - Ignace, R.

AU - Buemi, C. S.

AU - Umana, G.

AU - Ingallinera, A.

AU - Leone, F.

AU - Phillips, N. M.

AU - Agliozzo, C.

AU - Todt, H.

AU - Cerrigone, L.

PY - 2018/5/1

Y1 - 2018/5/1

N2 - We present new radio/millimeter measurements of the hot magnetic star HR5907 obtained with the VLA and ALMA interferometers. We find that HR5907 is the most radio luminous early type star in the cm-mm band among those presently known. Its multi-wavelength radio light curves are strongly variable with an amplitude that increases with radio frequency. The radio emission can be explained by the populations of the non-thermal electrons accelerated in the current sheets on the outer border of the magnetosphere of this fast-rotating magnetic star. We classify HR5907 as another member of the growing class of strongly magnetic fastrotating hot stars where the gyro-synchrotron emission mechanism efficiently operates in their magnetospheres. The new radio observations of HR5907 are combined with archival X-ray data to study the physical condition of its magnetosphere. The X-ray spectra of HR5907 show tentative evidence for the presence of non-thermal spectral component. We suggest that non-thermal X-rays originate a stellar X-ray aurora due to streams of non-thermal electrons impacting on the stellar surface. Taking advantage of the relation between the spectral indices of the X-ray power-law spectrum and the non-thermal electron energy distributions, we perform 3-D modelling of the radio emission for HR5907. The wavelength-dependent radio light curves probe magnetospheric layers at different heights above the stellar surface. A detailed comparison between simulated and observed radio light curves leads us to conclude that the stellar magnetic field of HR 5907 is likely non-dipolar, providing further indirect evidence of the complex magnetic field topology of HR5907.

AB - We present new radio/millimeter measurements of the hot magnetic star HR5907 obtained with the VLA and ALMA interferometers. We find that HR5907 is the most radio luminous early type star in the cm-mm band among those presently known. Its multi-wavelength radio light curves are strongly variable with an amplitude that increases with radio frequency. The radio emission can be explained by the populations of the non-thermal electrons accelerated in the current sheets on the outer border of the magnetosphere of this fast-rotating magnetic star. We classify HR5907 as another member of the growing class of strongly magnetic fastrotating hot stars where the gyro-synchrotron emission mechanism efficiently operates in their magnetospheres. The new radio observations of HR5907 are combined with archival X-ray data to study the physical condition of its magnetosphere. The X-ray spectra of HR5907 show tentative evidence for the presence of non-thermal spectral component. We suggest that non-thermal X-rays originate a stellar X-ray aurora due to streams of non-thermal electrons impacting on the stellar surface. Taking advantage of the relation between the spectral indices of the X-ray power-law spectrum and the non-thermal electron energy distributions, we perform 3-D modelling of the radio emission for HR5907. The wavelength-dependent radio light curves probe magnetospheric layers at different heights above the stellar surface. A detailed comparison between simulated and observed radio light curves leads us to conclude that the stellar magnetic field of HR 5907 is likely non-dipolar, providing further indirect evidence of the complex magnetic field topology of HR5907.

KW - Radio continuum: Stars

KW - Stars: Chemically peculiar

KW - Stars: Early-type

KW - Stars: Individual: HR 5907

KW - Stars: Magnetic field

KW - X-rays: Stars

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U2 - 10.1093/mnras/sty244

DO - 10.1093/mnras/sty244

M3 - Article

VL - 476

SP - 562

EP - 579

JO - Monthly Notices of the Royal Astronomical Society

JF - Monthly Notices of the Royal Astronomical Society

SN - 0035-8711

IS - 1

ER -