Zobrazeno 1 - 10
of 46
pro vyhledávání: '"R. Rothenflug"'
Autor:
J. Ballet, R. Rothenflug, Anne Decourchelle, P. Ferrando, Gloria Mabel Dubner, Elsa Beatriz Giacani
Publikováno v:
CONICET Digital (CONICET)
Consejo Nacional de Investigaciones Científicas y Técnicas
instacron:CONICET
Consejo Nacional de Investigaciones Científicas y Técnicas
instacron:CONICET
SN 1006 is the prototype of shell supernova remnants, in which non-thermal synchrotron emission dominates the X-ray spectrum. The non-thermal emission is due to the cosmic-ray electrons accelerated behind the blast wave. The X-ray synchrotron emissio
Autor:
R. Rothenflug
Publikováno v:
International Astronomical Union Colloquium. 115:146-155
The soft X-ray background is explained in terms of emission coming from hot gas. Most of these soft X-ray data were obtained by proportional counters with a poor energy resolution. Instruments having the capability to resolve lines were only flown by
Autor:
James Reeves, R. G. Griffiths, S. Dos Santos, C. V. Goodall, R. Lainé, William C. Priedhorsky, J. Clavel, S. Vercellone, Jean-François Hochedez, F. A. Cordova, L. Vigroux, Lothar Strüder, Joachim Trümper, P. Salvetat, F. A. Jansen, Simona Ghizzardi, Trevor J. Ponman, N. La Palombara, E. Kendziorra, Ulrich G. Briel, P. Dhez, Gabriele E. Villa, I. Butler, Keith O. Mason, Marco Barbera, J. L. Sauvageot, Martin J. L. Turner, D. Schmitt, Andrew D. Holland, R. Rothenflug, M. Boer, C. Pigot, A. Lagostina, M. Trifoglio, S. Molendi, Steven Sembay, P. Ferrando, Monique Arnaud, A. Short, P. J. Bennie, Claus Reppin, M. Lortholary, Martin Ward
This paper presents the XMM-Newton first-light observations of the Hickson-16 compact group of galaxies. Groups are possibly the oldest large-scale structures in the Universe, pre-dating clusters of galaxies, and are highly evolved. This group of sma
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::18cbfca2495ee3e413a2608bc619ea2d
http://arxiv.org/abs/astro-ph/0010612
http://arxiv.org/abs/astro-ph/0010612
Autor:
Richard G. West, T. Stadlbauer, Marc Audard, Steve Sembay, J. L. Sauvageot, Anne Decourchelle, R. Rothenflug, Bernd Aschenbach, J. Ballet
We present the observation of the Tycho supernova remnant obtained with the EPIC and RGS instruments onboard the XMM-Newton satellite. We compare images and azimuthally averaged radial profiles in emission lines from different elements (silicon and i
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::281d07bf85293589fc74628167f9f44b
Autor:
Guido Di Cocco, Salvatore Serio, S. Sciortino, John P. Pye, Ruediger Staubert, Richard E. Cole, Peter Predehl, Gabriele E. Villa, Andrew D. Holland, Gerald K. Skinner, B. H. Foing, P. A. Caraveo, Lothar Strueder, E. M. Quadrini, Trevor J. Ponman, L. Vigroux, Alan A. Wells, Gerhard Lutz, L. Koch, Giuseppe Bonelli, Ken Pounds, Claus Reppin, L. Chiappetti, Jean-Pierre Roques, Jean-Luc Atteia, Yvon Rio, Giovanni Peres, Giovanni F. Bignami, Joachim E. Truemper, Wolfgang Pietsch, C. V. Goodall, Jacky B. Cretolle, Claude Pigot, G. Boella, Pietro Ubertini, G. S. Vaiana, David H. Lumb, Eckhard Kendziorra, M. Trifoglio, Heinrich W. Braeuninger, Martin J. L. Turner, Alan H. Gabriel, A. P. Willmore, R. Rothenflug
Publikováno v:
SPIE Proceedings.
The capabilities of the European Photon Imaging Camera (EPIC), the main instrument of ESA's 'Cornerstone' mission in X-ray astronomy with multiple mirrors (XMM), are discussed. The CCD characteristics, spatial resolution, energy bandpass and faint so
Publikováno v:
International Astronomical Union Colloquium. 81:301-304
Soft X-ray surveys proved the existence of a local hot bubble surrounding the solar system (Mc Cammon et al 1983). Recently two experiments measured the spectrum of this hot interstellar medium with solid state detectors during rocket flights between
Autor:
R. Rocchia, M. Arnaud, C. Blondel, C. Cheron, J. C. Christy, L. Koch, R. Rothenflug, H. W. Schnopper, J. P. Delvaille
Publikováno v:
Symposium - International Astronomical Union. 101:357-360
In this paper, we present preliminary results of soft X-ray diffuse background observations. We observed two particular regions of the sky in the 0.3–1.5 keV range. The detection system consisted of three independent, 1 cm diameter, cooled solid st
Autor:
R. Rocchia, M. Arnaud, C. Blondel, C. Cheron, J. C. Christy, R. Ducros, L. Koch, R. Rothenflug, H. W. Schnopper, J. P. Delvaille
Publikováno v:
Space Science Reviews. 30:253-257
Publikováno v:
International Astronomical Union Colloquium. 101:411-414
We present the first results of an observational program of SNRs in the coronal lines of [FeX] and [FeXIV] using the Fabry-Perot spectrophotometer of the Observatoire de Marseille. These support previously published brightnesses.
Publikováno v:
Advances in Space Research. 2:233-236