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Formation of the Helium Line 10830 Å in Biconical Winds of Herbig Ae/Be Star. / Ermolaeva , T. A.; Grinin , V. P. ; Dmitriev , D. V.

Stars: From Collapse to Collapse, Proceedings of a conference held at Special Astrophysical Observatory, Nizhny Arkhyz, Russia 3-7 October 2016. Astronomical Society of the Pacific, 2017. p. 36 (Astronomical Society of the Pacific Conference Series; Vol. 510).

Research output: Chapter in Book/Report/Conference proceeding › Conference contribution › peer-review

Harvard

Ermolaeva , TA, Grinin , VP & Dmitriev , DV 2017, Formation of the Helium Line 10830 Å in Biconical Winds of Herbig Ae/Be Star. in Stars: From Collapse to Collapse, Proceedings of a conference held at Special Astrophysical Observatory, Nizhny Arkhyz, Russia 3-7 October 2016. Astronomical Society of the Pacific Conference Series, vol. 510, Astronomical Society of the Pacific, pp. 36, Stars: From Collapse to Collapse, Нижний Архыз, Russian Federation, 3/10/16.

APA

Ermolaeva , T. A., Grinin , V. P., & Dmitriev , D. V. (2017). Formation of the Helium Line 10830 Å in Biconical Winds of Herbig Ae/Be Star. In Stars: From Collapse to Collapse, Proceedings of a conference held at Special Astrophysical Observatory, Nizhny Arkhyz, Russia 3-7 October 2016 (pp. 36). (Astronomical Society of the Pacific Conference Series; Vol. 510). Astronomical Society of the Pacific.

Vancouver

Ermolaeva TA, Grinin VP, Dmitriev DV. Formation of the Helium Line 10830 Å in Biconical Winds of Herbig Ae/Be Star. In Stars: From Collapse to Collapse, Proceedings of a conference held at Special Astrophysical Observatory, Nizhny Arkhyz, Russia 3-7 October 2016. Astronomical Society of the Pacific. 2017. p. 36. (Astronomical Society of the Pacific Conference Series).

Author

Ermolaeva , T. A. ; Grinin , V. P. ; Dmitriev , D. V. / Formation of the Helium Line 10830 Å in Biconical Winds of Herbig Ae/Be Star. Stars: From Collapse to Collapse, Proceedings of a conference held at Special Astrophysical Observatory, Nizhny Arkhyz, Russia 3-7 October 2016. Astronomical Society of the Pacific, 2017. pp. 36 (Astronomical Society of the Pacific Conference Series).

BibTeX

@inproceedings{aefbfddd9edd426a93015fc4802d14d3,
title = "Formation of the Helium Line 10830 {\AA} in Biconical Winds of Herbig Ae/Be Star",
abstract = "Pre-main-sequence phase of stellar evolution is accompanied with the mass loss from young stars caused by the interaction between star and its surrounding environment. Mass loss in the form of different kinds of winds plays an important role in forming the emission spectra of stars. In this study we investigate the origin of the line He I 10830 {\AA} in biconical winds of Herbig Ae/Be stars. We consider two types of the wind: a hot wind (Te=106K) , and a“warm” wind (Te=9000-15000K) which is ionized by an X-ray emission. Calculations were performed using the microphysics code CLOUDY, version 13.03. It is shown, that “warm” wind model can explain the observed helium 10830 {\AA} line profiles.",
author = "Ermolaeva, {T. A.} and Grinin, {V. P.} and Dmitriev, {D. V.}",
year = "2017",
language = "English",
series = "Astronomical Society of the Pacific Conference Series",
publisher = "Astronomical Society of the Pacific",
pages = "36",
booktitle = "Stars: From Collapse to Collapse, Proceedings of a conference held at Special Astrophysical Observatory, Nizhny Arkhyz, Russia 3-7 October 2016",
address = "United States",
note = "null ; Conference date: 03-10-2016 Through 07-10-2016",
url = "https://www.sao.ru/",

}

RIS

TY - GEN

T1 - Formation of the Helium Line 10830 Å in Biconical Winds of Herbig Ae/Be Star

AU - Ermolaeva , T. A.

AU - Grinin , V. P.

AU - Dmitriev , D. V.

PY - 2017

Y1 - 2017

N2 - Pre-main-sequence phase of stellar evolution is accompanied with the mass loss from young stars caused by the interaction between star and its surrounding environment. Mass loss in the form of different kinds of winds plays an important role in forming the emission spectra of stars. In this study we investigate the origin of the line He I 10830 Å in biconical winds of Herbig Ae/Be stars. We consider two types of the wind: a hot wind (Te=106K) , and a“warm” wind (Te=9000-15000K) which is ionized by an X-ray emission. Calculations were performed using the microphysics code CLOUDY, version 13.03. It is shown, that “warm” wind model can explain the observed helium 10830 Å line profiles.

AB - Pre-main-sequence phase of stellar evolution is accompanied with the mass loss from young stars caused by the interaction between star and its surrounding environment. Mass loss in the form of different kinds of winds plays an important role in forming the emission spectra of stars. In this study we investigate the origin of the line He I 10830 Å in biconical winds of Herbig Ae/Be stars. We consider two types of the wind: a hot wind (Te=106K) , and a“warm” wind (Te=9000-15000K) which is ionized by an X-ray emission. Calculations were performed using the microphysics code CLOUDY, version 13.03. It is shown, that “warm” wind model can explain the observed helium 10830 Å line profiles.

UR - https://aspbooks.org/a/volumes/author_index/list_articles/?author=Ermolaeva%2C%20T.%20A.

UR - https://ui.adsabs.harvard.edu/abs/2017ASPC..510...36E/abstract

M3 - Conference contribution

T3 - Astronomical Society of the Pacific Conference Series

SP - 36

BT - Stars: From Collapse to Collapse, Proceedings of a conference held at Special Astrophysical Observatory, Nizhny Arkhyz, Russia 3-7 October 2016

PB - Astronomical Society of the Pacific

Y2 - 3 October 2016 through 7 October 2016

ER -

ID: 97764344