Zobrazeno 1 - 4
of 4
pro vyhledávání: '"Bailon, E. Jimenez"'
Autor:
Zelati, F. Coti, Baglio, M. C., Campana, S., D'Avanzo, P., Goldoni, P., Masetti, N., Muñoz-Darias, T., Covino, S., Fender, R. P., Bailón, E. Jiménez, Otí-Floranes, H., Palazzi, E., Ramón-Fox, F. G.
Publikováno v:
Monthly Notices of the Royal Astronomical Society, Volume 444, Issue 2, 21 October 2014, Pages 1783-1792
The binary millisecond radio pulsar PSR J1023+0038 has been recently the subject of multiwavelength monitoring campaigns which revealed that an accretion disc has formed around the neutron star (since 2013 June). We present here the results of X-ray
Externí odkaz:
http://arxiv.org/abs/1409.0427
Autor:
Zarattini, S., Barrena, R., Girardi, M., Castro-Rodriguez, N., Boschin, W., Aguerri, J. A. L., Méndez-Abreu, J., Sánchez-Janssen, R., Catalán-Torrecilla, C., Corsini, E. M., del Burgo, C., D'Onghia, E., Herrera-Ruiz, N., Iglesias-Páramo, J., Bailon, E. Jimenez, Muñoz, M. Lozada, Napolitano, N., Vilchez, J. M.
(Abridged) Fossil systems are group- or cluster-sized objects whose luminosity is dominated by a very massive central galaxy. In the current cold dark matter scenario, these objects formed hierarchically at an early epoch of the Universe and then slo
Externí odkaz:
http://arxiv.org/abs/1403.0588
We present results from a ~55 ks long XMM-Newton observation of the obscured AGN, NGC 5643, performed in July 2009. A previous, shorter (about 10 ks) XMM-Newton observation in February 2003 had left two major issues open, the nature of the hard X-ray
Externí odkaz:
http://arxiv.org/abs/1307.1591
Autor:
González, D. Rosa, Terlevich, E., Bailón, E. Jiménez, Terlevich, R., Ranalli, P., Comastri, A., Laird, E., Nandra, K.
In an effort to understand the correlation between X-ray emission and present star formation rate (SFR), we obtained XMM-Newton data to estimate the X-ray luminosities of a sample of actively starforming HII galaxies. The obtained X-ray luminosities
Externí odkaz:
http://arxiv.org/abs/0906.4461