Astronomy and Astrophysics – Astronomy
Scientific paper
Oct 2011
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011aspc..446..297a&link_type=abstract
Galaxy evolution: Infrared to millimeter wavelength perspective. Proceedings of a conference held at Guilin, China 25-29 October
Astronomy and Astrophysics
Astronomy
Scientific paper
Hereby we present an exploratory study of the surface brightness radial profiles (μ-r profiles hereafter) of massive (M˜>109.5 M&sun;) disk galaxies in the redshift range 0 ˜< z ˜< 1. We use recently acquired images from HST-WFC3 in the H160 band, and archive data from SDSS-DR7, to trace the rest-frame z' band at all redshifts. The comparison of average μ-r profiles, obtained from images with their spatial resolutions equaled, show no significant change in the explored range of redshifts, i. e. in the last ˜8 Gyr of cosmic time. The stellar surface density seems to be comparable, at equal fractions of the effective radius, and there is no evidence for the growth in relevance of bulges. At least not at the simulated resolution, which is 1.5 kpc (fwhm).
Azzollini Ruyman
Conselice Christopher J.
Trujillo Ignacio
No associations
LandOfFree
Evolution of the NIR Morphologies of Disk Galaxies since z˜1: A `Glance' into GOODS-South with HST-WFC3 does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with Evolution of the NIR Morphologies of Disk Galaxies since z˜1: A `Glance' into GOODS-South with HST-WFC3, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Evolution of the NIR Morphologies of Disk Galaxies since z˜1: A `Glance' into GOODS-South with HST-WFC3 will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1651129