3C 295: A Cluster and Its Cooling Flow atz= 0.46

نویسندگان

چکیده

برای دانلود باید عضویت طلایی داشته باشید

برای دانلود متن کامل این مقاله و بیش از 32 میلیون مقاله دیگر ابتدا ثبت نام کنید

اگر عضو سایت هستید لطفا وارد حساب کاربری خود شوید

منابع مشابه

3 C 295 , a Cluster and Its Cooling Flow at Z = 0 . 46

We present ROSAT HRI data of the distant and X-ray luminous (L x (bol) = 2.6 +0.4 −0.2 × 10 45 erg/sec) cluster of galaxies 3C 295. We fit both a one-dimensional and a two-dimensional isothermal β-model to the data, the latter one taking into account the effects of the point spread function (PSF). For the error analysis of the parameters of the two-dimensional model we introduce a Monte-Carlo t...

متن کامل

HRI observation of the cooling flow cluster

A ROSAT HRI observation of the cluster MS-0839.9+2938 at z=0.194 is presented. It confirms the earlier suggestion, based on the detection of extended Hα emission, that the inner regions of this cluster are dominated by a cooling flow. The surface brightness distribution within the cooling radius shows structures which can be interpreted as evidence of a highly inhomogeneous space distribution o...

متن کامل

Chandra Observation of the Cooling Flow Cluster

We present an analysis of the Chandra X-ray observation of A2052, including large-scale properties of the cluster as well as the central region, which includes the bright radio source 3C 317. We present temperature and abundance profiles using both projected and deprojected spectral analyses. The cluster shows the cooling flow signatures of excess surface brightness above a -model at the cluste...

متن کامل

A BeppoSAX observation of the cooling flow cluster Abell 2029

We present results from a BeppoSAX observation of the cooling flow cluster Abell 2029. The broad band spectrum (2–35 keV) of the cluster, when fitted with a model including a cooling flow component and a one temperature thermal component, yields a temperature of 8.3±0.2 keV and a metal abundance of 0.46±0.03 in solar units, for the latter. No evidence of a hard X-ray excess is found in the PDS ...

متن کامل

Cosmological MHD simulation of a cooling flow cluster

Context. Various observations of magnetic fields in the intra–cluster medium (ICM), most of the time restricted to cluster cores, point towards a field strength of a few μG (synchrotron radiation from radio relics and radio halos, inverse Compton radiation in X-rays and Faraday rotation measure of polarised background sources). Both the origin and the spatial structure of galaxy cluster magneti...

متن کامل

ذخیره در منابع من


  با ذخیره ی این منبع در منابع من، دسترسی به آن را برای استفاده های بعدی آسان تر کنید

ژورنال

عنوان ژورنال: The Astrophysical Journal

سال: 1999

ISSN: 0004-637X,1538-4357

DOI: 10.1086/307424