Sign on

SAO/NASA ADS Astronomy Abstract Service


· Find Similar Abstracts (with default settings below)
· Full Refereed Journal Article (PDF/Postscript)
· Full Refereed Scanned Article (GIF)
· References in the article
· Citations to the Article (90) (Citation History)
· Refereed Citations to the Article
· SIMBAD Objects (1)
· NED Objects (2)
· Also-Read Articles (Reads History)
·
· Translate This Page
Title:
Diffuse light in dense clusters of galaxies. I - R-band observations of Abell 2029
Authors:
Uson, Juan M.; Boughn, Stephen P.; Kuhn, Jeffrey R.
Affiliation:
AA(National Radio Astronomy Observatory, Socorro, NM), AB(Haverford College, PA), AC(Michigan State University, East Lansing)
Publication:
Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 369, March 1, 1991, p. 46-53. Research supported by NSF. (ApJ Homepage)
Publication Date:
03/1991
Category:
Astrophysics
Origin:
STI
NASA/STI Keywords:
Galactic Clusters, Galactic Mass, Intergalactic Media, Visual Photometry, Charge Coupled Devices, Galactic Evolution, Interacting Galaxies, Mass To Light Ratios
Astronomy Keywords:
cosmology, galaxies: clustering, galaxies: intergalactic medium, galaxies: photometry
DOI:
10.1086/169737
Bibliographic Code:
1991ApJ...369...46U

Abstract

We have developed an observing technique that uses a CCD detector, multiple overlapping exposures, and a tesselating algorithm that allows us to do reliable differential photometry over a large (about 0?6) field of view to a precision of 2 × 10-4 of the night-sky level, limited only by statistical noise.

We have measured the point-spread function of the telescope-detector combination out to 20' from the nominal pointing position. We have found that it is necessary to correct the data for the contamination from the extended halos of stars brighter than mR = 15.5 in order to measure diffuse light at levels below mu ˜ 26, or about 1 % of the average night-sky level.

We present R-band observations of the very dense cluster of galaxies Abell 2029. We detect an elliptical component of diffuse light extended halo of the cD galaxy with constant eccentricity of 0.9 that follows a de Vaucouleurs profile out to a distance of 425h 1; kpc [measured as d = (rminrmax)1/2]. The integrated luminosity of the cD galaxy with this halo is 5 × 1011h 2Lsun (R band).

The ratio of the diffuse light to the total cluster light in the elliptical annulus between d = 250h-1 kpc and d = 425h-1 kpc is 0.10±0.005, where the uncertainty comes mainly from the estimate of the contribution of the galaxies. We place an upper limit of 5% to the ratio of diffuse light to total cluster light in the elliptical annulus between d = 425h-1kpc and d = 850h-1kpc.


Printing Options

Print whole paper
Print Page(s) through

Return 600 dpi PDF to Acrobat/Browser. Different resolutions (200 or 600 dpi), formats (Postscript, PDF, etc), page sizes (US Letter, European A4, etc), and compression (gzip,compress,none) can be set through the Printing Preferences



More Article Retrieval Options

HELP for Article Retrieval


Bibtex entry for this abstract   Preferred format for this abstract (see Preferences)

  New!

Find Similar Abstracts:

Use: Authors
Title
Keywords (in text query field)
Abstract Text
Return: Query Results Return    items starting with number
Query Form
Database: Astronomy
Physics
arXiv e-prints