Disc wind in the HH 30 binary models › Научные исследования в СПбГУ

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Disc wind in the HH 30 binary models. / Tambovtseva, L. V.; Grinin, V. P.

в: Monthly Notices of the Royal Astronomical Society, Том 387, № 3, 07.2008, стр. 1313-1317.

Результаты исследований: Научные публикации в периодических изданиях › статья › Рецензирование

Harvard

Tambovtseva, LV & Grinin, VP 2008, 'Disc wind in the HH 30 binary models', Monthly Notices of the Royal Astronomical Society, Том. 387, № 3, стр. 1313-1317. https://doi.org/10.1111/j.1365-2966.2008.13329.x

APA

Tambovtseva, L. V., & Grinin, V. P. (2008). Disc wind in the HH 30 binary models. Monthly Notices of the Royal Astronomical Society, 387(3), 1313-1317. https://doi.org/10.1111/j.1365-2966.2008.13329.x

Vancouver

Tambovtseva LV, Grinin VP. Disc wind in the HH 30 binary models. Monthly Notices of the Royal Astronomical Society. 2008 Июль;387(3):1313-1317. https://doi.org/10.1111/j.1365-2966.2008.13329.x

Author

Tambovtseva, L. V. ; Grinin, V. P. / Disc wind in the HH 30 binary models. в: Monthly Notices of the Royal Astronomical Society. 2008 ; Том 387, № 3. стр. 1313-1317.

BibTeX

@article{65d470d3d9064b7183a5f35853d047a3,

title = "Disc wind in the HH 30 binary models",

abstract = "Recent interferometric observations of the young stellar object (YSO) HH 30 have revealed a low-velocity outflow in the 12CO J=1-2 molecule line. We present here two models of the low-velocity disc winds with the aim of investigating the origin of this molecular outflow. Following Andlada et al., we treated HH 30 as a binary system. Two cases have been considered: (i) the orbital period P = 53 yr and (ii) P ≤ 1 yr. Calculations showed that in the first case the outflow cone had a spiral-like structure due to summing the velocities of the orbital motion and the disc wind. Such a structure contradicts the observations. In the second case, the outflow cone demonstrates a symmetry relatively to the system axis and agrees well with the observations.",

keywords = "Binaries: close, Circumstellar matter, Stars: individual: HH 30",

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

year = "2008",

month = jul,

doi = "10.1111/j.1365-2966.2008.13329.x",

language = "English",

volume = "387",

pages = "1313--1317",

journal = "Monthly Notices of the Royal Astronomical Society",

issn = "0035-8711",

publisher = "Wiley-Blackwell",

number = "3",

}

RIS

TY - JOUR

T1 - Disc wind in the HH 30 binary models

AU - Tambovtseva, L. V.

AU - Grinin, V. P.

PY - 2008/7

Y1 - 2008/7

N2 - Recent interferometric observations of the young stellar object (YSO) HH 30 have revealed a low-velocity outflow in the 12CO J=1-2 molecule line. We present here two models of the low-velocity disc winds with the aim of investigating the origin of this molecular outflow. Following Andlada et al., we treated HH 30 as a binary system. Two cases have been considered: (i) the orbital period P = 53 yr and (ii) P ≤ 1 yr. Calculations showed that in the first case the outflow cone had a spiral-like structure due to summing the velocities of the orbital motion and the disc wind. Such a structure contradicts the observations. In the second case, the outflow cone demonstrates a symmetry relatively to the system axis and agrees well with the observations.

AB - Recent interferometric observations of the young stellar object (YSO) HH 30 have revealed a low-velocity outflow in the 12CO J=1-2 molecule line. We present here two models of the low-velocity disc winds with the aim of investigating the origin of this molecular outflow. Following Andlada et al., we treated HH 30 as a binary system. Two cases have been considered: (i) the orbital period P = 53 yr and (ii) P ≤ 1 yr. Calculations showed that in the first case the outflow cone had a spiral-like structure due to summing the velocities of the orbital motion and the disc wind. Such a structure contradicts the observations. In the second case, the outflow cone demonstrates a symmetry relatively to the system axis and agrees well with the observations.

KW - Binaries: close

KW - Circumstellar matter

KW - Stars: individual: HH 30

UR - http://www.scopus.com/inward/record.url?scp=45249098220&partnerID=8YFLogxK

U2 - 10.1111/j.1365-2966.2008.13329.x

DO - 10.1111/j.1365-2966.2008.13329.x

M3 - Article

AN - SCOPUS:45249098220

VL - 387

SP - 1313

EP - 1317

JO - Monthly Notices of the Royal Astronomical Society

JF - Monthly Notices of the Royal Astronomical Society

SN - 0035-8711

IS - 3

ER -

ID: 87425143