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X-ray emission from Ae/Be Herbig stars due to disc-stellar magnetosphere interaction. / Холтыгин, Александр Федорович; Рыспаева, Е.Б.; Maxim, Lyutikov.

In: Monthly Notices of the Royal Astronomical Society, Vol. 521, No. 2, 14.03.2023, p. 2427-2438.

Research output: Contribution to journal › Article › peer-review

Harvard

Холтыгин, АФ, Рыспаева, ЕБ & Maxim, L 2023, 'X-ray emission from Ae/Be Herbig stars due to disc-stellar magnetosphere interaction', Monthly Notices of the Royal Astronomical Society, vol. 521, no. 2, pp. 2427-2438. https://doi.org/10.1093/mnras/stad629

APA

Холтыгин, А. Ф., Рыспаева, Е. Б., & Maxim, L. (2023). X-ray emission from Ae/Be Herbig stars due to disc-stellar magnetosphere interaction. Monthly Notices of the Royal Astronomical Society, 521(2), 2427-2438. https://doi.org/10.1093/mnras/stad629

Vancouver

Холтыгин АФ, Рыспаева ЕБ, Maxim L. X-ray emission from Ae/Be Herbig stars due to disc-stellar magnetosphere interaction. Monthly Notices of the Royal Astronomical Society. 2023 Mar 14;521(2):2427-2438. https://doi.org/10.1093/mnras/stad629

Author

Холтыгин, Александр Федорович ; Рыспаева, Е.Б. ; Maxim, Lyutikov. / X-ray emission from Ae/Be Herbig stars due to disc-stellar magnetosphere interaction. In: Monthly Notices of the Royal Astronomical Society. 2023 ; Vol. 521, No. 2. pp. 2427-2438.

BibTeX

@article{b1b798b0bde34a3f9e892a4ccc5bc249,
title = "X-ray emission from Ae/Be Herbig stars due to disc-stellar magnetosphere interaction",
abstract = "We reanalyse archival X-ray data of 16 Ae/Be Herbig stars obtained by the XMM-Newton and Chandra satellites. Stellar X-ray spectra in the energy range 0.2-8 keV were fitted with the use of APEC and MEKAL hot plasma emission models, and with models with an additional power-law component. We find that for Herbig stars, the dependence of the unabsorbed X-ray luminosity on stellar mass and radius, LX ∝ RαMβ with α ≈ 3 and β ≈ 2, is similar to that for T Tauri stars. The independently determined accretion rates, rotation periods, and the surface magnetic fields follow a tight correlation predicted by the standard magnetospheric accretion theory. We suggest that X-ray emission from Herbig stars is powered by magnetic reconnection events in the tenuous corona at the disc-magnetosphere boundary.",
author = "Холтыгин, {Александр Федорович} and Е.Б. Рыспаева and Lyutikov Maxim",
year = "2023",
month = mar,
day = "14",
doi = "10.1093/mnras/stad629",
language = "English",
volume = "521",
pages = "2427--2438",
journal = "Monthly Notices of the Royal Astronomical Society",
issn = "0035-8711",
publisher = "Wiley-Blackwell",
number = "2",

}

RIS

TY - JOUR

T1 - X-ray emission from Ae/Be Herbig stars due to disc-stellar magnetosphere interaction

AU - Холтыгин, Александр Федорович

AU - Рыспаева, Е.Б.

AU - Maxim, Lyutikov

PY - 2023/3/14

Y1 - 2023/3/14

N2 - We reanalyse archival X-ray data of 16 Ae/Be Herbig stars obtained by the XMM-Newton and Chandra satellites. Stellar X-ray spectra in the energy range 0.2-8 keV were fitted with the use of APEC and MEKAL hot plasma emission models, and with models with an additional power-law component. We find that for Herbig stars, the dependence of the unabsorbed X-ray luminosity on stellar mass and radius, LX ∝ RαMβ with α ≈ 3 and β ≈ 2, is similar to that for T Tauri stars. The independently determined accretion rates, rotation periods, and the surface magnetic fields follow a tight correlation predicted by the standard magnetospheric accretion theory. We suggest that X-ray emission from Herbig stars is powered by magnetic reconnection events in the tenuous corona at the disc-magnetosphere boundary.

AB - We reanalyse archival X-ray data of 16 Ae/Be Herbig stars obtained by the XMM-Newton and Chandra satellites. Stellar X-ray spectra in the energy range 0.2-8 keV were fitted with the use of APEC and MEKAL hot plasma emission models, and with models with an additional power-law component. We find that for Herbig stars, the dependence of the unabsorbed X-ray luminosity on stellar mass and radius, LX ∝ RαMβ with α ≈ 3 and β ≈ 2, is similar to that for T Tauri stars. The independently determined accretion rates, rotation periods, and the surface magnetic fields follow a tight correlation predicted by the standard magnetospheric accretion theory. We suggest that X-ray emission from Herbig stars is powered by magnetic reconnection events in the tenuous corona at the disc-magnetosphere boundary.

UR - https://ui.adsabs.harvard.edu/abs/2023MNRAS.521.2427R/abstract

UR - https://www.mendeley.com/catalogue/93129059-711a-3365-96c0-b5117bee1d28/

U2 - 10.1093/mnras/stad629

DO - 10.1093/mnras/stad629

M3 - Article

VL - 521

SP - 2427

EP - 2438

JO - Monthly Notices of the Royal Astronomical Society

JF - Monthly Notices of the Royal Astronomical Society

SN - 0035-8711

IS - 2

ER -

ID: 104089991