Infrared emission from M31

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Abstract

view Abstract Citations (100) References (18) Co-Reads Similar Papers Volume Content Graphics Metrics Export Citation NASA/ADS Infrared emission from M31. Habing, H. J. ; Miley, G. ; Young, E. ; Baud, B. ; Boggess, N. ; Clegg, P. E. ; de Jong, T. ; Harris, S. ; Raimond, E. ; Rowan-Robinson, M. ; Soifer, B. T. Abstract Maps of M31 have been obtained at wavelengths of 12, 25, 60, and 100 microns. Emission is detected from the center and from a ring of 50 arcmin radius. The ring is that also seen in H I, in H II, and in radio continuum radiation. The spectrum of the central emission suggests a hotter dust temperature than in the ring. M31 is a weak infrared source, the radiation measured longward of 12 microns being only 3 percent of its total luminosity. The two closest companion galaxies, M32 and NGC 205, have also been detected. Publication: The Astrophysical Journal Pub Date: March 1984 DOI: 10.1086/184223 Bibcode: 1984ApJ...278L..59H Keywords: Andromeda Galaxy; Astronomical Maps; Galactic Radiation; Infrared Astronomy; Spaceborne Astronomy; Emission Spectra; Hydrogen Clouds; Infrared Astronomy Satellite; Spectral Bands; Astrophysics full text sources ADS | data products NED (4) SIMBAD (3)

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