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Low Surface Brightness Galaxies Beyond Z = 0.5: Existence, Detection and Properties

Published online by Cambridge University Press:  12 April 2016

G. Bothun*
Affiliation:
Dept. of Physics, University of Oregon, Eugene OR 97403, [email protected]

Abstract

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I argue that low surface brightness disks evolve sufficiently slowly that, at any redshift, there should be a high space density of these objects. Cosmological dimming, in combination with the tenacity of Freeman’s Law, will make their direct detection very difficult. Given their abundance at z =0, it seems reasonable to suggest that such hidden galaxies will be important absorbers along the line of sight to distant QSOs.

Type
Properties of Low Surface Brightness galaxies
Copyright
Copyright © Astronomical Society of the Pacific 1999

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