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19942004
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astro-ph2004

2-100 keV Spectrum of an Actively Star Forming Galaxy

Massimo Persic, Yoel Rephaeli

We compute the synthetic 2-100 keV spectrum of an actively star forming galaxy. To this aim we use a luminosity function of point sources appropriate for starbursts (based on Chand…

astro-ph2003

The Ultra Luminous Infrared Galaxy MKN 231: New clues from BeppoSAX and XMM-Newton

V. Braito, R. Della Ceca, E. Piconcelli +11

We present BeppoSAX and XMM-Newton observations of MKN 231. These observations and in particular the BeppoSAX PDS data allowed us to unveil, for the first time, the highly absorbed…

astro-ph2002

An XMM-Newton Survey of Ultra-Luminous Infrared Galaxies

V. Braito, A. Franceschini, R. Della Ceca +8

We present preliminary results of XMM-Newton observations of 5 Ultra-luminous Infrared Galaxies (ULIRGs), part of a mini-survey program dedicated to 10 ULIRGs selected from the bri…

astro-ph1999

BeppoSAX uncovers a type-2 QSO in the hyperluminous infrared galaxy IRAS 09104+4109

A. Franceschini, L. Bassani, L. Cappi +4

We studied with BeppoSAX the infrared luminous galaxy IRAS 09104+4109 over a very wide X-ray band from 0.1 to 80 keV. Our observations indicate the dominance of a thermal component…

astro-ph1997

Dark Matter Halos around Galaxies

Paolo Salucci, Massimo Persic

We present evidence that all galaxies, of any Hubble type and luminosity, bear the kinematical signature of a mass component distributed differently from the luminous matter. We re…

astro-ph1996

Dark Baryons in the Universe: the Quest Goes On

Paolo Salucci, Massimo Persic

We show that the high local baryonic fraction, M(bar) ~ 1/3 M(tot), found in groups and clusters of galaxies does not reconcile the observed cosmological baryon density with the st…