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Chandra Tutorial Eleonora Torresi + Giorgio Lanzuisi // + Fabio Vito + Cristian Vignali , , + Giulia Migliori bssc (3) issue 10 iv table of contents xml browsers 23 publishing software 23 archiving, storage and retrieval software 23 security tools 19 INAF – IASFBO, via P. Gobetti , Bologna, Italy 20 Kapteyn Astronomical Institute, University of Groningen, AV Groningen, The Netherlands Received 20 July /Accepted 28 September ABSTRACT bltadwin.ru chemical evolution of galaxies on a cosmological timescale is still a matter of debate despite the increasing number of.

We review the high energy properties of Misaligned AGNs associated with gamma-ray sources detected by Fermi in 24 months of survey. Most of them are nearby emission low power radio galaxies (i.e FRIs) which probably have structured jets. On the contrary, high power radio sources (i.e FRIIs) with GeV emission are rare. The small number of FRIIs does not seem to be related to their higher. Internal Report IASF-BO / Free-free spectral distortions amplified by a non negligible density contrast of the intergalactic medium T. Trombetti1 and C. Burigana1,2 1INAF-IASF Bologna, Via Piero Gobetti , I, Bologna, Italy 2Dipartimento di Fisica e Scienze della Terra, Universita` degli Studi di Ferrara, Via Giuseppe Saragat 1, I Ferrara, Italy. One of the main debated astrophysical problems is the role of the AGN feedback in galaxy formation. It is known that massive black holes have a profound effect on the formation and evolution of galaxies, but how black holes and galaxies communicate is still an unsolved problem. For Radio Galaxies, feedback studies have mainly focused on jet/cavity systems in the most massive and X-ray luminous.

Ref.: EGOS-MCS-S2K-ICD Issue: 6. 7DraftA Date: SCOS Database Import ICD Page: vii ESA/OPS-GIC Abstract This document is the interface control document of the data import into SCOS run-time database. → How to download X-ray data from a public archive → How the downloaded files look like → How to reduce X-ray (Chandra) data → How to create the radio and/or X-ray contours for an extended object. dof=degrees of freedom=number of datapoints – number of free parameters= == Χ2/dof close to unity means that it is a good fit (not in this case!) Null hypothesis probability=probability that the model is correct for those datapoints (if close to 1) All the adopted models should be physically motivated according to the.