Brackett γ radiation from the inner gaseous accretion disk, magnetosphere, and disk wind region of Herbig AeBe stars

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Brackett γ radiation from the inner gaseous accretion disk, magnetosphere, and disk wind region of Herbig AeBe stars. / Tambovtseva, L. V.; Grinin, V. P.; Weigelt, G.

In: Astronomy and Astrophysics, Vol. 590, A97, 2016.

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

BibTeX

@article{3bf281985ef54787bfe1fc6082dd2f93,

title = "Brackett γ radiation from the inner gaseous accretion disk, magnetosphere, and disk wind region of Herbig AeBe stars",

abstract = "Various disk and outflow components such as the magnetosphere, the disk wind, the gaseous accretion disk, and other regions may contribute to the hydrogen line emission of young Herbig AeBe stars. Non-LTE modeling was performed to show the influence of the model parameters of each emitting region on the intensity and shape of the Brγ line profile, to present the spatial brightness distribution of each component, and to compare the contribution of each component to the total line emission. The modeling shows that the disk wind is the dominant contributor to the Brγ line rather than the magnetosphere and inner gaseous accretion disk. The contribution of the disk wind region to the Hα line is also considered.",

keywords = "Accretion, accretion disks, Radiative transfer, Stars: pre-main sequence, Stars: variables: T Tauri, Herbig Ae/Be, Stars: winds, outflows, Techniques: spectroscopic",

author = "Tambovtseva, {L. V.} and Grinin, {V. P.} and G. Weigelt",

note = "Publisher Copyright: {\textcopyright} 2016 ESO.",

year = "2016",

doi = "10.1051/0004-6361/201628256",

language = "English",

volume = "590",

journal = "ASTRONOMY & ASTROPHYSICS",

issn = "0004-6361",

publisher = "EDP Sciences",

}

RIS

TY - JOUR

T1 - Brackett γ radiation from the inner gaseous accretion disk, magnetosphere, and disk wind region of Herbig AeBe stars

AU - Tambovtseva, L. V.

AU - Grinin, V. P.

AU - Weigelt, G.

PY - 2016

Y1 - 2016

N2 - Various disk and outflow components such as the magnetosphere, the disk wind, the gaseous accretion disk, and other regions may contribute to the hydrogen line emission of young Herbig AeBe stars. Non-LTE modeling was performed to show the influence of the model parameters of each emitting region on the intensity and shape of the Brγ line profile, to present the spatial brightness distribution of each component, and to compare the contribution of each component to the total line emission. The modeling shows that the disk wind is the dominant contributor to the Brγ line rather than the magnetosphere and inner gaseous accretion disk. The contribution of the disk wind region to the Hα line is also considered.

AB - Various disk and outflow components such as the magnetosphere, the disk wind, the gaseous accretion disk, and other regions may contribute to the hydrogen line emission of young Herbig AeBe stars. Non-LTE modeling was performed to show the influence of the model parameters of each emitting region on the intensity and shape of the Brγ line profile, to present the spatial brightness distribution of each component, and to compare the contribution of each component to the total line emission. The modeling shows that the disk wind is the dominant contributor to the Brγ line rather than the magnetosphere and inner gaseous accretion disk. The contribution of the disk wind region to the Hα line is also considered.

KW - Accretion, accretion disks

KW - Radiative transfer

KW - Stars: pre-main sequence

KW - Stars: variables: T Tauri, Herbig Ae/Be

KW - Stars: winds, outflows

KW - Techniques: spectroscopic

UR - http://www.scopus.com/inward/record.url?scp=84971278376&partnerID=8YFLogxK

U2 - 10.1051/0004-6361/201628256

DO - 10.1051/0004-6361/201628256

M3 - Article

AN - SCOPUS:84971278376

VL - 590

JO - ASTRONOMY & ASTROPHYSICS

JF - ASTRONOMY & ASTROPHYSICS

SN - 0004-6361

M1 - A97

ER -

ID: 87424465