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dc.contributor.authorAbolins, J.A.
dc.contributor.authorAdams, D.J.
dc.contributor.authorJameson, R.F.
dc.contributor.authorHough, J.
dc.contributor.authorAxon, D.J.
dc.identifier.citationAbolins , J A , Adams , D J , Jameson , R F , Hough , J & Axon , D J 1979 , ' Detection of a bright ridge in the 2.2 MU-M emission of M82 ' , Monthly Notices of the Royal Astronomical Society , vol. 186 , no. 3 , pp. 23-27 .
dc.identifier.otherPURE: 160662
dc.identifier.otherPURE UUID: 78b4fb26-e532-4368-a5c4-6ef0c58435cc
dc.identifier.otherdspace: 2299/3217
dc.descriptionOriginal article can be found via: Copyright Royal Astronomical Society [Full text of this article is not available in the UHRA]
dc.description.abstractPhotometric 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.en
dc.relation.ispartofMonthly Notices of the Royal Astronomical Society
dc.titleDetection of a bright ridge in the 2.2 MU-M emission of M82en
dc.contributor.institutionSchool of Physics, Astronomy and Mathematics
dc.description.statusPeer reviewed
dc.relation.schoolSchool of Physics, Astronomy and Mathematics
rioxxterms.typeJournal Article/Review

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