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E. Pian – LNGS, 13 Sep 2005 Elena Pian - INAF, Trieste Astronomical Observatory, Italy LNGS Summer Institute 2005 GRB: Modern Status.
Documents E. Pian – LNGS, 13 Sep 2005 Elena Pian - INAF, Trieste Astronomical Observatory, Italy LNGS Summer...

Slide 1E. Pian – LNGS, 13 Sep 2005 Elena Pian - INAF, Trieste Astronomical Observatory, Italy LNGS Summer Institute 2005 GRB: Modern Status Slide 2 E. Pian – LNGS, 13…

Radio Loud AGN in 2XMMi Multi-wavelength view A. Labiano (ESAC-ESA), M. Guainazzi (ESAC-ESA), S. Bianchi (Rome-3), G. Miniutti (CAB-INTA)
Documents Radio Loud AGN in 2XMMi Multi-wavelength view A. Labiano (ESAC-ESA), M. Guainazzi (ESAC-ESA), S....

Slide 1 Radio Loud AGN in 2XMMi Multi-wavelength view A. Labiano (ESAC-ESA), M. Guainazzi (ESAC-ESA), S. Bianchi (Rome-3), G. Miniutti (CAB-INTA) Slide 2 CAIXA Catalogue…

Suzaku Results of SN 1006: Chemical abundances of the youngest Galactic Type Ia Supernova Remnant Katsuji Koyama Department of physics, Kyoto University,
Documents Suzaku Results of SN 1006: Chemical abundances of the youngest Galactic Type Ia Supernova Remnant...

Slide 1Suzaku Results of SN 1006: Chemical abundances of the youngest Galactic Type Ia Supernova Remnant Katsuji Koyama Department of physics, Kyoto University, Kitashirakawa,…

The XMM-Newton hard band wide angle Survey Nicoletta Carangelo and Silvano Molendi (IASF-MI(CNR)) Epic Consortium Meeting Palazzo Steri, Palermo, 14-16.
Documents The XMM-Newton hard band wide angle Survey Nicoletta Carangelo and Silvano Molendi (IASF-MI(CNR))...

Slide 1 The XMM-Newton hard band wide angle Survey Nicoletta Carangelo and Silvano Molendi (IASF-MI(CNR)) Epic Consortium Meeting Palazzo Steri, Palermo, 14-16 October 2003…

The goal of the study : To localize sources of the quasi-stationary slow solar wind. Method:
Documents The goal of the study : To localize sources of the quasi-stationary slow solar wind. Method:

PROBA 2 Guest Investigator project (2010-2012) EUV imaging of the solar corona and study of slow solar wind streams V. Slemzin1, L. Harra2, S. Kuzin1, A. Urnov1, F. Goryaev1,…

BLACK HOLE
Documents BLACK HOLE

BLACK HOLE Movie courtesy Wolfgang Steffen, University Guadalajara, Mexico QUASAR-MICROQUASAR ANALOGY The scales of length and time are proportional to MBH Rsh = 2GMBH/c2…

NASSP Masters 5003F - Computational Astronomy - 2009 Lecture 21 6.4 keV Fe line and the Kerr metric Satellite observatories –Attitude and boresight X-ray.
Documents NASSP Masters 5003F - Computational Astronomy - 2009 Lecture 21 6.4 keV Fe line and the Kerr metric....

NASSP Masters 5003F - Computational Astronomy - 2009 Lecture 21 6.4 keV Fe line and the Kerr metric Satellite observatories Attitude and boresight X-ray instrumentation and…

Element spots in HgMn stars Heidi Korhonen Centre for Star and Planet Formation & Niels Bohr Institute University of Copenhagen.
Documents Element spots in HgMn stars Heidi Korhonen Centre for Star and Planet Formation & Niels Bohr...

Element spots in HgMn stars Heidi Korhonen Centre for Star and Planet Formation & Niels Bohr Institute University of Copenhagen Outline General properties of HgMn stars…

The Star Formation Histories of Red Sequence Galaxies Mike Hudson U. Waterloo / IAP Steve Allanson (Waterloo) Allanson, MH et al 09, ApJ 702, 1275 Russell.
Documents The Star Formation Histories of Red Sequence Galaxies Mike Hudson U. Waterloo / IAP Steve Allanson.....

The Star Formation Histories of Red Sequence Galaxies Mike Hudson U. Waterloo / IAP Steve Allanson (Waterloo) Allanson, MH et al 09, ApJ 702, 1275 Russell Smith (Durham)…

Element spots in HgMn stars
Documents Element spots in HgMn stars

Element spots in HgMn stars Heidi Korhonen Centre for Star and Planet Formation & Niels Bohr Institute University of Copenhagen Outline General properties of HgMn stars…

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