The infrared (H) surface brightness of galaxies as a function of the morphological type

Details The infrared (H) surface brightness of galaxies as a function of the morphological type The infrared (H) surface brightness of galaxies as a function of the morphological type

May 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986a%26a...160..331m&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 160, no. 2, May 1986, p. 331-334.

Astronomy and Astrophysics

Astronomy

1

Brightness, Galactic Structure, Infrared Astronomy, Galactic Radiation, Magnitude, Morphology, Surface Properties

Scientific paper

The total IR surface brightness of galaxies of different morphological type is presently computed on the basis of H(0.5) magnitudes and UGC diameters. A strong correlation is noted betwen the IR brightness thus determined and the galaxy morphological type. It is suggested that the IR surface brightness changes by about 2.5 mag along the Hubble sequence.

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