期刊
ASTROPHYSICAL JOURNAL LETTERS
卷 679, 期 2, 页码 L69-L72出版社
IOP PUBLISHING LTD
DOI: 10.1086/589283
关键词
galaxies : evolution; galaxies : high-redshift; galaxies : structure
We present deep color profiles for a sample of 415 disk galaxies within the redshift range, and 0.1 < z <= 1.1 contained in HST ACS imaging of the GOODS-South field. For each galaxy, passband combinations are chosen to obtain, at each redshift, the best possible approximation to the rest-frame u - g color. We find that objects which show a truncation in their stellar disk ( type II objects) usually show a minimum in their color profile at the break, or very near to it, with a maximum to minimum amplitude in color of less than or similar to 0.2 mag arcsec(-2), a feature which is persistent through the explored range of redshifts (i.e., in the last similar to 8 Gyr). This color structure is in qualitative agreement with recent model expectations where the break of the surface brightness profiles is the result of the interplay between a radial star formation cutoff and a redistribution of stellar mass by secular processes.
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