Spectropolarimetry of the molecular-hydrogen line emission from OMC-1

M. Burton; J. Hough; D.J. Axon; T. Hasegawa; M. Tamura; M.J. McCaughrean; I. McLean

Spectropolarimetry of the molecular-hydrogen line emission from OMC-1

M. Burton, J. Hough, D.J. Axon, T. Hasegawa, M. Tamura, M.J. McCaughrean, I. McLean

Centre for Astrophysics Research (CAR)

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

Abstract

Observations of the H2 v = 1-0 S(1) line at 35 km/s velocity resolution were obtained at several locations within OMC-1, including the molecular hydrogen reflection nebula. All line profiles are smooth and show no evidence for being composed of discrete components. The data are discussed with respect to a model for the H2 line formation in which the emission originates in discrete clumps moving at different velocities. It is suggested that the extended blue wing may come from fast-moving clumps embedded in a wind.

Original language	English
Pages (from-to)	161-174
Journal	Monthly Notices of the Royal Astronomical Society
Volume	235
Issue number	1
Publication status	Published - 1988

Cite this

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title = "Spectropolarimetry of the molecular-hydrogen line emission from OMC-1",

abstract = "Observations of the H2 v = 1-0 S(1) line at 35 km/s velocity resolution were obtained at several locations within OMC-1, including the molecular hydrogen reflection nebula. All line profiles are smooth and show no evidence for being composed of discrete components. The data are discussed with respect to a model for the H2 line formation in which the emission originates in discrete clumps moving at different velocities. It is suggested that the extended blue wing may come from fast-moving clumps embedded in a wind.",

author = "M. Burton and J. Hough and D.J. Axon and T. Hasegawa and M. Tamura and M.J. McCaughrean and I. McLean",

note = "Copyright Royal Astronomical Society. [Full text of this article is not available in the UHRA]",

year = "1988",

language = "English",

volume = "235",

pages = "161--174",

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

issn = "0035-8711",

publisher = "Oxford University Press (OUP)",

number = "1",

}

TY - JOUR

T1 - Spectropolarimetry of the molecular-hydrogen line emission from OMC-1

AU - Burton, M.

AU - Hough, J.

AU - Axon, D.J.

AU - Hasegawa, T.

AU - Tamura, M.

AU - McCaughrean, M.J.

AU - McLean, I.

N1 - Copyright Royal Astronomical Society. [Full text of this article is not available in the UHRA]

PY - 1988

Y1 - 1988

N2 - Observations of the H2 v = 1-0 S(1) line at 35 km/s velocity resolution were obtained at several locations within OMC-1, including the molecular hydrogen reflection nebula. All line profiles are smooth and show no evidence for being composed of discrete components. The data are discussed with respect to a model for the H2 line formation in which the emission originates in discrete clumps moving at different velocities. It is suggested that the extended blue wing may come from fast-moving clumps embedded in a wind.

AB - Observations of the H2 v = 1-0 S(1) line at 35 km/s velocity resolution were obtained at several locations within OMC-1, including the molecular hydrogen reflection nebula. All line profiles are smooth and show no evidence for being composed of discrete components. The data are discussed with respect to a model for the H2 line formation in which the emission originates in discrete clumps moving at different velocities. It is suggested that the extended blue wing may come from fast-moving clumps embedded in a wind.

M3 - Article

SN - 0035-8711

VL - 235

SP - 161

EP - 174

JO - Monthly Notices of the Royal Astronomical Society

JF - Monthly Notices of the Royal Astronomical Society

IS - 1

ER -

Spectropolarimetry of the molecular-hydrogen line emission from OMC-1

Abstract

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