Published in "Photometric Redshifts and the Detection of High Redshift Galaxies", ASP Conference Series, Vol. 191, 1999. Edited by Ray Weymann, Lisa Storrie-Lombardi, Marcin Sawicki, and Robert Brunner.
Abstract. The increased incidence of morphologically peculiar
galaxies at faint
magnitudes in the optical could be attributable either to
"morphological k-corrections" (the change in appearance when viewing
high-z objects at shorter rest-frame wavelengths), or an increase in
the incidence of truly irregular systems with redshift. The deep,
high-resolution GTO-NICMOS near-IR imaging of a portion of the northern
Hubble Deep Field has been combined with the WFPC2 data and
photometric redshift estimates to study the redshift evolution of
morphology, comparing galaxy appearance at the same rest-wavelengths
(Bunker, Spinrad & Thompson 1999).
It appears that morphological
k-corrections are only significant in a minority of cases, and that
once these are accounted for, evolution is still demanded - galaxies
were smaller and more irregular in the past, with some of the
peculiarities probably merger-related. This multi-waveband data set also
enables a study of the spatially-resolved stellar populations in distant
galaxies. A near-infrared analysis of some of the brighter spirals
shows more pronounced barred structure than in the optical, indicating
that the apparent decline in barred spirals at faint magnitudes in the
optical HDF may be due to band-shifting effects at the higher redshifts,
rather than intrinsic evolution.
Key Words:
galaxies: evolution -- galaxies: fundamental parameters
(classification) -- galaxies: interactions -- galaxies: irregular
-- galaxies: peculiar -- infrared: galaxies
For a postscript version of the article, click
here.
GALAXY MORPHOLOGY IN
THE GTO-NICMOS NORTHERN HUBBLE DEEP FIELD
Andrew J. Bunker 1
NICMOS Postdoctoral Research Fellow,
Dept. of Astronomy,
U.C. Berkeley,
601 Campbell Hall, Berkeley CA94720
E-mail:
bunker@bigz.berkeley.edu
1 In collaboration with Hyron Spinrad (Department of
Astronomy, U.C. Berkeley),
Rodger Thompson (Steward Observatory, University of Arizona) and the
NICMOS-GTO team.