Zobrazeno 1 - 10
of 73
pro vyhledávání: '"Avillez, M."'
Autor:
Sasaki, M., Haberl, F., Henze, M., Saeedi, S., Williams, B. F., Plucinsky, P. P., Hatzidimitriou, D., Karampelas, A., Sokolovsky, K. V., Breitschwerdt, D., de Avillez, M. A., Filipovic, M. D., Galvin, T., Kavanagh, P. J., Long, K. S.
Publikováno v:
A&A 620, A28 (2018)
We carried out new observations of two fields in the northern ring of M31 with XMM-Newton with two exposures of 100 ks each and obtained a complete list of X-ray sources down to a sensitivity limit of ~7 x 10^34 erg s^-1 (0.5 - 2.0 keV). The major ob
Externí odkaz:
http://arxiv.org/abs/1809.08020
Autor:
Delabrouille, J., de Bernardis, P., Bouchet, F. R., Achúcarro, A., Ade, P. A. R., Allison, R., Arroja, F., Artal, E., Ashdown, M., Baccigalupi, C., Ballardini, M., Banday, A. J., Banerji, R., Barbosa, D., Bartlett, J., Bartolo, N., Basak, S., Baselmans, J. J. A., Basu, K., Battistelli, E. S., Battye, R., Baumann, D., Benoît, A., Bersanelli, M., Bideaud, A., Biesiada, M., Bilicki, M., Bonaldi, A., Bonato, M., Borrill, J., Boulanger, F., Brinckmann, T., Brown, M. L., Bucher, M., Burigana, C., Buzzelli, A., Cabass, G., Cai, Z. -Y., Calvo, M., Caputo, A., Carvalho, C. -S., Casas, F. J., Castellano, G., Catalano, A., Challinor, A., Charles, I., Chluba, J., Clements, D. L., Clesse, S., Colafrancesco, S., Colantoni, I., Contreras, D., Coppolecchia, A., Crook, M., D'Alessandro, G., D'Amico, G., da Silva, A., de Avillez, M., de Gasperis, G., De Petris, M., de Zotti, G., Danese, L., Désert, F. -X., Desjacques, V., Di Valentino, E., Dickinson, C., Diego, J. M., Doyle, S., Durrer, R., Dvorkin, C., Eriksen, H. -K., Errard, J., Feeney, S., Fernández-Cobos, R., Finelli, F., Forastieri, F., Franceschet, C., Fuskeland, U., Galli, S., Génova-Santos, R. T., Gerbino, M., Giusarma, E., Gomez, A., González-Nuevo, J., Grandis, S., Greenslade, J., Goupy, J., Hagstotz, S., Hanany, S., Handley, W., Henrot-Versillé, S., Hernández-Monteagudo, C., Hervias-Caimapo, C., Hills, M., Hindmarsh, M., Hivon, E., Hoang, D. T., Hooper, D. C., Hu, B., Keihänen, E., Keskitalo, R., Kiiveri, K., Kisner, T., Kitching, T., Kunz, M., Kurki-Suonio, H., Lagache, G., Lamagna, L., Lapi, A., Lasenby, A., Lattanzi, M., Brun, A. M. C. Le, Lesgourgues, J., Liguori, M., Lindholm, V., Lizarraga, J., Luzzi, G., Macìas-Pérez, J. F., Maffei, B., Mandolesi, N., Martin, S., Martinez-Gonzalez, E., Martins, C. J. A. P., Masi, S., Massardi, M., Matarrese, S., Mazzotta, P., McCarthy, D., Melchiorri, A., Melin, J. -B., Mennella, A., Mohr, J., Molinari, D., Monfardini, A., Montier, L., Natoli, P., Negrello, M., Notari, A., Noviello, F., Oppizzi, F., O'Sullivan, C., Pagano, L., Paiella, A., Pajer, E., Paoletti, D., Paradiso, S., Partridge, R. B., Patanchon, G., Patil, S. P., Perdereau, O., Piacentini, F., Piat, M., Pisano, G., Polastri, L., Polenta, G., Pollo, A., Ponthieu, N., Poulin, V., Prêle, D., Quartin, M., Ravenni, A., Remazeilles, M., Renzi, A., Ringeval, C., Roest, D., Roman, M., Roukema, B. F., Rubino-Martin, J. -A., Salvati, L., Scott, D., Serjeant, S., Signorelli, G., Starobinsky, A. A., Sunyaev, R., Tan, C. Y., Tartari, A., Tasinato, G., Toffolatti, L., Tomasi, M., Torrado, J., Tramonte, D., Trappe, N., Triqueneaux, S., Tristram, M., Trombetti, T., Tucci, M., Tucker, C., Urrestilla, J., Väliviita, J., Van de Weygaert, R., Van Tent, B., Vennin, V., Verde, L., Vermeulen, G., Vielva, P., Vittorio, N., Voisin, F., Wallis, C., Wandelt, B., Wehus, I., Weller, J., Young, K., Zannoni, M.
Future observations of cosmic microwave background (CMB) polarisation have the potential to answer some of the most fundamental questions of modern physics and cosmology. In this paper, we list the requirements for a future CMB polarisation survey ad
Externí odkaz:
http://arxiv.org/abs/1706.04516
Autor:
Aharonian, F., Arshakian, T. G., Allen, B., Banerjee, R., Beck, R., Becker, W., Bomans, D. J., Breitschwerdt, D., Brüggen, M., Brunthaler, A., Catinella, B., Champion, D., Ciardi, B., Crocker, R., de Avillez, M. A., Dettmar, R. J., Engels, D., Enßlin, T., Enke, H., Fieseler, T., Gizon, L., Hackmann, E., Hartmann, B., Henkel, C., Hoeft, M., Iapichino, L., Innes, D., James, C., Jasche, J., Jones, D., Kagramanova, V., Kauffmann, G., Keane, E., Kerp, J., Klöckner, H. -R., Kokkotas, K., Kramer, M., Krause, M., Krupp, N., Kunz, J., Lämmerzahl, C., Lee, K. J., List, M., Liu, K., Lobanov, A., Mann, G., Merloni, A., Middelberg, E., Niemeyer, J., Noutsos, A., Perlick, V., Reich, W., Richter, P., Roy, A., Saintonge, A., Schäfer, G., Schaffner-Bielich, J., Schinnerer, E., Schleicher, D., Schneider, P., Schwarz, D. J., Sedrakian, A., Sesana, A., Smolčić, V., Solanki, S., Tuffs, R., Vetter, M., Weber, E., Weller, J., Wex, N., Wucknitz, O., Zwaan, M.
The Square Kilometre Array (SKA) is the most ambitious radio telescope ever planned. With a collecting area of about a square kilometre, the SKA will be far superior in sensitivity and observing speed to all current radio facilities. The scientific c
Externí odkaz:
http://arxiv.org/abs/1301.4124
Until recently the dynamical evolution of the interstellar medium (ISM) was simulated using collisional ionization equilibrium (CIE) conditions. However, the ISM is a dynamical system, in which the plasma is naturally driven out of equilibrium due to
Externí odkaz:
http://arxiv.org/abs/1301.2890
Using three-dimensional non-equilibrium ionization (NEI) hydrodynamical simulation of the interstellar medium (ISM), we study the electron density, $n_{e}$, in the Galactic disk and compare it with the values derived from dispersion measures towards
Externí odkaz:
http://arxiv.org/abs/1204.1511
Autor:
The COrE Collaboration, Armitage-Caplan, C., Avillez, M., Barbosa, D., Banday, A., Bartolo, N., Battye, R., Bernard, JP., de Bernardis, P., Basak, S., Bersanelli, M., Bielewicz, P., Bonaldi, A., Bucher, M., Bouchet, F., Boulanger, F., Burigana, C., Camus, P., Challinor, A., Chongchitnan, S., Clements, D., Colafrancesco, S., Delabrouille, J., De Petris, M., De Zotti, G., Dickinson, C., Dunkley, J., Ensslin, T., Fergusson, J., Ferreira, P., Ferriere, K., Finelli, F., Galli, S., Garcia-Bellido, J., Gauthier, C., Haverkorn, M., Hindmarsh, M., Jaffe, A., Kunz, M., Lesgourgues, J., Liddle, A., Liguori, M., Lopez-Caniego, M., Maffei, B., Marchegiani, P., Martinez-Gonzalez, E., Masi, S., Mauskopf, P., Matarrese, S., Melchiorri, A., Mukherjee, P., Nati, F., Natoli, P., Negrello, M., Pagano, L., Paoletti, D., Peacocke, T., Peiris, H., Perroto, L., Piacentini, F., Piat, M., Piccirillo, L., Pisano, G., Ponthieu, N., Rath, C., Ricciardi, S., Martin, J. Rubino, Salatino, M., Shellard, P., Stompor, R., Urrestilla, L. Toffolatti J., Van Tent, B., Verde, L., Wandelt, B., Withington, S.
COrE (Cosmic Origins Explorer) is a fourth-generation full-sky, microwave-band satellite recently proposed to ESA within Cosmic Vision 2015-2025. COrE will provide maps of the microwave sky in polarization and temperature in 15 frequency bands, rangi
Externí odkaz:
http://arxiv.org/abs/1102.2181
We review the evolution of the interstellar medium in disc galaxies, and show, both analytically and by numerical 3D hydrodynamic simulations, that the disc-halo connection is an essential ingredient in understanding the evolution of star forming gal
Externí odkaz:
http://arxiv.org/abs/0905.0431
Autor:
de Avillez, M. A., Breitschwerdt, D.
The supernova-driven interstellar medium in star-forming galaxies has Reynolds numbers of the order of $10^{6}$ or even larger. We study, by means of adaptive mesh refinement hydro- and magnetohydrodynamical simulations that cover the full available
Externí odkaz:
http://arxiv.org/abs/astro-ph/0611307
Publikováno v:
Mon.Not.Roy.Astron.Soc.373:993-1003,2006
We present a new unbiased search and analysis of all B stars in the solar neighbourhood (within a volume of 400 pc diameter) using the Arivel data base to track down the remains of the OB associations, which hosted the supernovae responsible for the
Externí odkaz:
http://arxiv.org/abs/astro-ph/0609227
State of the art models of the ISM use adaptive mesh refinement to capture small scale structures, by refining on the fly those regions of the grid where density and pressure gradients occur, keeping at the same time the existing resolution in the ot
Externí odkaz:
http://arxiv.org/abs/astro-ph/0502078