Detection of a bright ridge in the 2.2 MU-M emission of M82

J.A. Abolins; D.J. Adams; R.F. Jameson; J. Hough; D.J. Axon

Detection of a bright ridge in the 2.2 MU-M emission of M82

J.A. Abolins, D.J. Adams, R.F. Jameson, J. Hough, D.J. Axon

Centre for Astrophysics Research (CAR)

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Abstract

Photometric scans through the central region of M82 with a resolution of 6 arcsec reveal that the 2.2-micron emission source has a compact ridge structure which is approximately aligned + or - 10 deg with the major axis of the galaxy. The source has an integrated K magnitude of 6.5 and dimensions of 300 x 75 pc, corresponding to 20 x 5 arcsec on the sky. The 2.2-micron ridge embraces the bright visible knots A and E and lies close to the center of the 10-micron emission region and the subarcsecond radio source.

Original language	English
Pages (from-to)	23-27
Journal	Monthly Notices of the Royal Astronomical Society
Volume	186
Issue number	3
Publication status	Published - 1979

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@article{78b4fb26e5324368a5c46ef0c58435cc,

title = "Detection of a bright ridge in the 2.2 MU-M emission of M82",

abstract = "Photometric scans through the central region of M82 with a resolution of 6 arcsec reveal that the 2.2-micron emission source has a compact ridge structure which is approximately aligned + or - 10 deg with the major axis of the galaxy. The source has an integrated K magnitude of 6.5 and dimensions of 300 x 75 pc, corresponding to 20 x 5 arcsec on the sky. The 2.2-micron ridge embraces the bright visible knots A and E and lies close to the center of the 10-micron emission region and the subarcsecond radio source.",

author = "J.A. Abolins and D.J. Adams and R.F. Jameson and J. Hough and D.J. Axon",

note = "Original article can be found via: http://cdsads.u-strasbg.fr/ Copyright Royal Astronomical Society [Full text of this article is not available in the UHRA]",

year = "1979",

language = "English",

volume = "186",

pages = "23--27",

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

issn = "0035-8711",

publisher = "Oxford University Press (OUP)",

number = "3",

}

TY - JOUR

T1 - Detection of a bright ridge in the 2.2 MU-M emission of M82

AU - Abolins, J.A.

AU - Adams, D.J.

AU - Jameson, R.F.

AU - Hough, J.

AU - Axon, D.J.

N1 - Original article can be found via: http://cdsads.u-strasbg.fr/ Copyright Royal Astronomical Society [Full text of this article is not available in the UHRA]

PY - 1979

Y1 - 1979

N2 - Photometric scans through the central region of M82 with a resolution of 6 arcsec reveal that the 2.2-micron emission source has a compact ridge structure which is approximately aligned + or - 10 deg with the major axis of the galaxy. The source has an integrated K magnitude of 6.5 and dimensions of 300 x 75 pc, corresponding to 20 x 5 arcsec on the sky. The 2.2-micron ridge embraces the bright visible knots A and E and lies close to the center of the 10-micron emission region and the subarcsecond radio source.

AB - Photometric scans through the central region of M82 with a resolution of 6 arcsec reveal that the 2.2-micron emission source has a compact ridge structure which is approximately aligned + or - 10 deg with the major axis of the galaxy. The source has an integrated K magnitude of 6.5 and dimensions of 300 x 75 pc, corresponding to 20 x 5 arcsec on the sky. The 2.2-micron ridge embraces the bright visible knots A and E and lies close to the center of the 10-micron emission region and the subarcsecond radio source.

M3 - Article

SN - 0035-8711

VL - 186

SP - 23

EP - 27

JO - Monthly Notices of the Royal Astronomical Society

JF - Monthly Notices of the Royal Astronomical Society

IS - 3

ER -

Detection of a bright ridge in the 2.2 MU-M emission of M82

Abstract

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