We use cookies to ensure that we give you the best experience on our website. By continuing to browse this repository, you give consent for essential cookies to be used. You can read more about our Privacy and Cookie Policy.

Durham Research Online
You are in:

The x-ray evolution of early-type galaxies in the extended Chandra Deep Field-South.

Lehmer, B. D. and Brandt, W. N. and Alexander, D. M. and Bell, E. F. and McIntosh, D. H. and Bauer, F. E. and Hasinger, G. and Mainieri, V. and Miyaji, T. and Schneider, D. P. and Steffen, A. T. (2007) 'The x-ray evolution of early-type galaxies in the extended Chandra Deep Field-South.', Astrophysical journal., 657 (1). pp. 681-699.


We investigate the evolution over the last 6.3 Gyr of cosmic time (i.e., since ) of the average X‐ray properties of early‐type galaxies within the Extended Chandra Deep Field–South (E‐CDF‐S). Our early‐type galaxy sample includes 539 objects with red sequence colors and Sérsic indices larger than , which were selected jointly from the COMBO‐17 (Classifying Objects by Medium‐Band Observations in 17 Filters) and GEMS (Galaxy Evolution from Morphologies and SEDs) surveys. We utilize the deep Chandra observations over the E‐CDF‐S and X‐ray stacking analyses to constrain primarily the average X‐ray emission from ``normal'' early‐type galaxies (i.e., those that are not dominated by luminous AGNs). We study separately optically luminous () and faint () galaxy samples, which we expect to have soft (0.5–2.0 keV) X‐ray emission dominated by hot (1 keV) interstellar gas and low‐mass X‐ray binary (LMXB) populations, respectively. The AGN fraction of our optically luminous sample evolves with redshift in a manner consistent with the evolution observed in other investigations of X‐ray–selected AGNs. We find that the X‐ray–to–B‐band mean luminosity ratio () for normal optically luminous galaxies does not evolve significantly over . This lack of X‐ray evolution implies a general balance between the heating and cooling of the hot gas. If transient AGN activity is largely responsible for maintaining this balance, then we infer that mechanical power must be dominating the feedback out to . Furthermore, in this scenario the average mechanical AGN power must remain roughly constant over the last half of cosmic time. For our optically faint early‐type galaxies, we find suggestive evidence that increases with redshift over.

Item Type:Article
Keywords:Cosmology, Observations, Galaxies, Active, Elliptical and Lenticular, cD, Surveys, X-rays.
Full text:PDF - Published Version (1020Kb)
Publisher Web site:
Publisher statement:© 2007. The American Astronomical Society. All rights reserved.
Record Created:21 Jan 2008
Last Modified:12 Aug 2014 11:40

Social bookmarking: del.icio.usConnoteaBibSonomyCiteULikeFacebookTwitterExport: EndNote, Zotero | BibTex
Usage statisticsLook up in GoogleScholar | Find in a UK Library