Caught in the act: The identification of the galaxies responsible for the faint blue excess

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dc.creatorDriver, Simon P.
dc.creatorWindhorst, Rogier A.
dc.creatorGriffiths, Richard E.
dc.date1995-11-28
dc.date.accessioned2026-07-07T02:20:29Z
dc.date.available2026-07-07T02:20:29Z
dc.descriptionWe summarise recent Hubble Space Telescope results on the morphology of faint field galaxies. Our two principle results are: (1) the galaxies responsible for the faint blue excess have late-type/irregular morphology and (2) the number counts of normal galaxies, ellipticals and early-type spirals, are well fit by standard no-evolution models implying that the giant population was in place and mature by a redshift of $\ge 0.7$.
dc.descriptionTo be published in Proceedings of IAU symposium 171, "New light on Galaxy Evolution", Eds.: R.Bender and R. Davies, 4 pages of gzip compressed and uuencoded postscript. Also available at http://www.phys.unsw.edu.au/~spd/bib.html
dc.identifierhttps://arxiv.org/abs/astro-ph/9511135
dc.identifierhttp://arxiv.org/abs/astro-ph/9511135
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/10227
dc.subjectAstrophysics
dc.titleCaught in the act: The identification of the galaxies responsible for the faint blue excess
dc.typetext

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