Photometry of seven clusters of galaxies at intermediate redshift

E. Molinari; A. Buzzoni; G. Chincarini

doi:10.1051/aas:1996254

Free Access

Issue		Astron. Astrophys. Suppl. Ser. Volume 119, Number 3, November I 1996


Page(s)		391 - 401
DOI		https://doi.org/10.1051/aas:1996254
Published online		15 November 1996

Astron. Astrophys. Suppl. Ser. 119, 391-401 (1996)

Photometry of seven clusters of galaxies at intermediate redshift $Mathematical equation: $^{(z = 0.15 \div 0.50)}$$ ^*

E. Molinari¹, A. Buzzoni¹^,2 and G. Chincarini¹^,3

¹ Osservatorio Astronomico di Brera, Via Bianchi, 46 22055 Merate (Lc), Italy
² Visiting astronomer at the INAOE, A.P. 51, 72000 Puebla, Mexico
³ Università degli Studi, Via Celoria, 16 20133 Milano, Italy e-mail: This email address is being protected from spambots. You need JavaScript enabled to view it.

Send offprint request to: E. Molinari

Received: 11 January 1996
Accepted: 15 March 1996

Abstract

Gunn g, r, i photometry for the 7 clusters MRC0254-274, Cl0317+15, MS0418.3-3844, Cl1141-283, A1689, A3594, S0781B is presented. For each cluster we derived the spatial distribution properties obtaining the core radius and the concentration parameters. Color properties of the cluster galaxy population are also briefly discussed. 

Key words: galaxies: clusters: genaral / galaxies: photometry

Based on observations made at the European Southern Observatory (ESO), La Silla, Chile

Photometry of seven clusters of galaxies at intermediate redshift *

Photometry of seven clusters of galaxies at intermediate redshift $Mathematical equation: $^{(z = 0.15 \div 0.50)}$$ ^*