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On the Assembly History of Early-Type Galaxies in the Hubble Deep Field-North
Author(s) -
Pieter van Dokkum,
Richard S. Ellis
Publication year - 2003
Publication title -
the astrophysical journal
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 2.376
H-Index - 489
eISSN - 1538-4357
pISSN - 0004-637X
DOI - 10.1086/377680
Subject(s) - physics , astrophysics , redshift , galaxy , elliptical galaxy , fundamental plane (elliptical galaxies) , astronomy , balmer series , galaxy group , lenticular galaxy , spectral line , emission spectrum
We present deep Keck spectroscopy for a sample of I<22.5 field early-typegalaxies selected morphologically in the redshift range 0.56=0.88. However, we find enhanced Hdelta absorption of equivalent width 4.0 Angstrom in the mean spectrum of theten galaxies, indicating the presence of young stars. We infer that thegalaxies have composite stellar populations, consisting of a low mass youngcomponent in addition to a dominating old component. As the bulk of the stellarmass must have formed at z >~ 2 our results argue against formation scenariosinvolving major mergers of gas-rich disk systems at 1

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