Zobrazeno 1 - 10
of 145
pro vyhledávání: '"G C, Palumbo"'
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 419:321-329
We review the soft X-ray properties of 3C 390.3, 3C 120, 3C 382 and 3C 445, the only Broad Line Radio Galaxies (BLRG) for which good quality gratings data are currently available. The XMM-Newton/RGS data of 3C 390.3 and 3C 120 were re-analyzed search
Autor:
Giorgio G. C. Palumbo
Publikováno v:
Nuclear Physics B - Proceedings Supplements. :34-49
The first attempt by Italian scientists to carry on Astrophysical observations from Space can be traced back to the early 60ʼs just after the launch of the first satellites. Dominated by Physicists for decades, slowly space astrophysics has become o
Autor:
Giorgio G. C. Palumbo, Anna Lia Longinotti, Matteo Guainazzi, A. A. Nucita, Eleonora Torresi, Francesco Tombesi, Paola Grandi
Publikováno v:
Monthly Notices of the Royal Astronomical Society: Letters. 401:L10-L14
Recent high-resolution measurements suggest that the soft X-ray spectrum of obscured Radio Galaxies (RG) exhibits signatures of photoionised gas (e.g. 3C 445 and 3C 33) similar to those observed in radio-quiet obscured Active Galactic Nuclei (AGN). W
Autor:
Paola Grandi, T. Kawaguchi, N. Cappelluti, T. J. L. Courvoisier, Giuseppe Malaguti, G. Di Cocco, J. Rodriguez, Luis C. Ho, Luigi Foschini, Ken Ebisawa, Giorgio G. C. Palumbo
Publikováno v:
Advances in Space Research. 38(7):1378-1381
著者人数:11名
Accepted: 2005-06-13
資料番号: SA1000579000
Accepted: 2005-06-13
資料番号: SA1000579000
Autor:
Paola Marziani, M. Cappi, Giorgio G. C. Palumbo, Loredana Bassani, Guido Risaliti, Alberto Franceschini, M. Salvati, Enrico Piconcelli, V. Braito, K. Iwasawa, Massimo Persic, Paola Severgnini, R. Della Ceca, Giuseppe Malaguti
Publikováno v:
Nuclear Physics B - Proceedings Supplements. 132:153-156
We present BeppoSAX and XMM-Newton observations of Mrk 231. These observations and in particular the BeppoSAX PDS data allowed us to unveil, for the first time, the highly absorbed (NH∼2×1024 cm−2) AGN component. We find that: a) the AGN powerin
Autor:
G. Vedrenne, A. J. Dean, W. Hermsen, Niels Lund, Christoph Winkler, Bonnard J. Teegarden, Neil Gehrels, P. Ubertini, R. A. Sunyaev, J. A. Paul, A. Giménez, J. M. Mas-Hesse, V. Schönfelder, Thierry J.-L. Courvoisier, G. Di Cocco, Francois Lebrun, J. P. Roques, S. A. Grebenev, Giorgio G. C. Palumbo, Herbert W. Schnopper
Publikováno v:
Astronomy & Astrophysics. 411:L1-L6
The ESA observatory INTEGRAL (International Gamma-Ray Astrophysics Laboratory) is dedicated to the fine spectroscopy (2.5 keV FWHM @ 1 MeV) and fine imaging (angular resolution: 12 arcmin FWHM) of celestial gamma-ray sources in the energy range 15 ke
Autor:
G. G. C. Palumbo, Giovanni F. Bignami
Publikováno v:
Advances in Space Research. 31:327-330
In the framework of a five year plan the Italian Space Agency has started a national program of small scientific satellites. The first two, AGILE and DAVID are already at an advanced stage of development. The former is dedicated to Gamma Ray Astrophy
Autor:
M. Cappi, M. Dadina, L. Maraschi, Loredana Bassani, Massimo Persic, P. O. Petrucci, Lucía Ballo, Giuseppe Malaguti, R. Della Ceca, Giorgio G. C. Palumbo, Alberto Franceschini, Fabrizio Tavecchio
Publikováno v:
The Astrophysical Journal. 581:L9-L13
Using a long (150 ks) broadband (0.1-40 keV) BeppoSAX observation of the merging starburst system Arp 299 (=IC 694 + NGC 3690), we found the first unambiguous evidence of the presence of a deeply buried (NH 2.5 × 1024 cm-2) active galactic nucleus (
Autor:
M. Orsini, C. Maxia, R. L. Sorochenko, Stefano Cortiglioni, S. Poppi, A. P. Tsivilev, Giorgio G. C. Palumbo
Publikováno v:
Astronomical & Astrophysical Transactions. 20:197-201
Publikováno v:
International Astronomical Union Colloquium. 174:90-99
A method of searching for multiplets in a large catalogue of galaxies with measured redshifts is described. Compact Groups samples having different local and global characteristics are generated when the algorithm is applied to ZCAT catalogue. Both l