INAF – Osservatorio Astronomico di Trieste C. Morossi Chemical evolution in the Universe: the next 30 years 16-20 Sept, 2013 Castiglione della Pescaia,
INAF – Osservatorio Astronomico di Bologna Technology Introduction.
The hard X-ray spectrum of Pulsar Wind Nebulae Data-models comparison in the Simbol-X era F. Bocchino, INAF Osservatorio Astronomico di Palermo with contributions.
The Role of Clays in Shielding DNA against X-Ray Radiation: Possible Implications on the origin of life Angela Ciaravella F. Scappini (2), M. Franchi (3),
Bocchino ea08a
Evidence ofr mature_bulges_and_an_inside_out_quenching_phase_3_billion_years_after_the_big_bang
Nustar reveals extreme_absortion_in_z_05_type_2_quasars
P. Saracco 1 M. Longhetti 1, A. Gargiulo 1 1 INAF – Osservatorio Astronomico di Brera, Milano Italy Galaxy Evolution and Environment - Bologna, November.
ASCI/Alliances Center for Astrophysical Thermonuclear Flashes Evaporation of Clouds in Thermally Conducting, Radiative Supernova Remnants S. Orlando (1),
Astronomy and Astrophysics Cluster in EGEE-III
Imaging: intensity and magnetic measurements
The hard X-ray spectrum of Pulsar Wind Nebulae