Università di Roma Tor Vergata & INAF-IASF Roma [email protected].
ASTR112 The Galaxy Lecture 7 Prof. John Hearnshaw 11. The galactic nucleus and central bulge 11.1 Infrared observations (cont.) 11.2 Radio observations.
Radio Measurements of the Height of Strong Coronal Magnetic Fields Above Spots at the Limb Jeff Brosius (Catholic Univ.) Stephen White (Univ. of MD)
Massive Objects at the Centers of Galaxies Roger Blandford KIPAC Stanford.
RXJ0146.9 +6121 a soft X-ray excess in a low luminosity accreting pulsar La Palombara & Mereghetti astro-ph/0604193.
Observations and NLFFF Modeling of AR 10953
Lyndsay Fletcher, University of Glasgow Ramaty High Energy Solar Spectroscopic Imager Fast Particles in Solar Flares The view from RHESSI (and TRACE) MRT.
Cataclysmic variables as hard X-ray emitters seen by INTEGRAL The X-ray Universe 2008, Granada, Spain, 27-30 May R. Gális 1,2, R. Hudec 1, F. Münz 3, M.
An XMM-Newton spatially resolved study of metal abundance evolution in distant galaxy clusters
R. Hudec, V. Šimon F. Munz, J. Štrobl, P. Kubánek, P. Sobotka, R. Urban Astronomical Institute, Academy of Sciences 251 65 Ondrejov, Czech Republic & ISDC,
Hard X-ray and radio observations of the 3 June 2007 flare Nicole Vilmer Meriem Alaoui Abdallaoui Solar Activity during the Onset of Solar Cycle 24 8-12.
Giuseppina Coppola1 First predicted by the Russian scientists Sunayaev and Zel’dovich in 1969. Galaxy Clusters have hot gas that produce electrons by bremsstahlung.
