Mon. Not. R. Astron. Soc., 426, 1731-1749 (2012/November-1)
The galaxy ancestor problem.
DISNEY M.J. and LANG R.H.
Abstract (from CDS):
The Hubble Space Telescope (HST) finds galaxies whose Tolman dimming exceeds 10mag. Could evolution alone explain these as our ancestor galaxies or could they be representatives of quite a different dynasty whose descendants are no longer prominent today? We explore the latter hypothesis and argue that surface brightness selection effects naturally bring into focus quite different dynasties from different redshifts. Thus, the HST z = 7 galaxies could be examples of galaxies whose descendants are both too small and too choked with dust to be recognizable in our neighbourhood easily today. Conversely, the ancestors of the Milky Way and its obvious neighbours would have completely sunk below the sky at z > 1.2, unless they were more luminous in the past, although their diffused light could account for the missing re-ionization flux. This Succeeding Prominent Dynasties Hypothesis (SPDH) fits the existing observations both naturally and well even without evolution, including the bizarre distributions of galaxy surface brightness found in deep fields, the angular size ∼ (1 + z)–1 law, `downsizing' which turns out to be an `illusion' in the sense that it does not imply evolution, `infant mortality', that is, the discrepancy between stars born and stars seen, the existence of `red nuggets', and finally the recently discovered and unexpected excess of quasar absorption line damped Lyα systems at high redshift. If galaxies were not significantly brighter in the past and the SPDH were true, then a large proportion of galaxies could remain sunk from sight, possibly at all redshifts, and these sunken galaxies could supply the missing re-ionization flux. We show that fishing these sunken galaxies out of the sky by their optical emissions alone is practically impossible, even when they are nearby. More ingenious methods are needed to detect them. It follows that disentangling galaxy evolution through studying ever higher redshift galaxies may be a forlorn hope because one could be comparing young oranges with old apples, not ancestors with their true descendants.
© 2012 The Authors Monthly Notices of the Royal Astronomical Society © 2012 RAS
galaxies: evolution - galaxies: high-redshift - galaxies: ISM - quasars: absorption lines - galaxies: statistics - dark ages, reionization, first stars
View the reference in ADS
To bookmark this query, right click on this link: simbad:2012MNRAS.426.1731D and select 'bookmark this link' or equivalent in the popup menu