Zobrazeno 1 - 10
of 512
pro vyhledávání: '"A. Decourchelle"'
While Tycho's supernova remnant is one of the most studied type Ia Galactic supernova remnants, a global view of the physical properties of its ejecta is lacking, to understand its mysteries. In particular, the spatial distribution of the Si-rich eje
Externí odkaz:
http://arxiv.org/abs/2404.17296
Publikováno v:
A&A 680, A80 (2023)
450 years after the explosion of the Type Ia SN1572, the dynamics of the Tycho supernova remnant can give us keys to understand the explosion mechanism and the interaction of the remnant with the interstellar medium. To probe the asymmetries and the
Externí odkaz:
http://arxiv.org/abs/2309.01621
Autor:
Barret, Didier, Albouys, Vincent, Herder, Jan-Willem den, Piro, Luigi, Cappi, Massimo, Huovelin, Juhani, Kelley, Richard, Mas-Hesse, J. Miguel, Paltani, Stéphane, Rauw, Gregor, Rozanska, Agata, Svoboda, Jiri, Wilms, Joern, Yamasaki, Noriko, Audard, Marc, Bandler, Simon, Barbera, Marco, Barcons, Xavier, Bozzo, Enrico, Ceballos, Maria Teresa, Charles, Ivan, Costantini, Elisa, Dauser, Thomas, Decourchelle, Anne, Duband, Lionel, Duval, Jean-Marc, Fiore, Fabrizio, Gatti, Flavio, Goldwurm, Andrea, Hartog, Roland den, Jackson, Brian, Jonker, Peter, Kilbourne, Caroline, Korpela, Seppo, Macculi, Claudio, Mendez, Mariano, Mitsuda, Kazuhisa, Molendi, Silvano, Pajot, François, Pointecouteau, Etienne, Porter, Frederick, Pratt, Gabriel W., Prêle, Damien, Ravera, Laurent, Sato, Kosuke, Schaye, Joop, Shinozaki, Keisuke, Skup, Konrad, Soucek, Jan, Thibert, Tanguy, Vink, Jacco, Webb, Natalie, Chaoul, Laurence, Raulin, Desi, Simionescu, Aurora, Torrejon, Jose Miguel, Acero, Fabio, Branduardi-Raymont, Graziella, Ettori, Stefano, Finoguenov, Alexis, Grosso, Nicolas, Kaastra, Jelle, Mazzotta, Pasquale, Miller, Jon, Miniutti, Giovanni, Nicastro, Fabrizio, Sciortino, Salvatore, Yamaguchi, Hiroya, Beaumont, Sophie, Cucchetti, Edoardo, D'Andrea, Matteo, Eckart, Megan, Ferrando, Philippe, Kammoun, Elias, Lotti, Simone, Mesnager, Jean-Michel, Natalucci, Lorenzo, Peille, Philippe, de Plaa, Jelle, Ardellier, Florence, Argan, Andrea, Bellouard, Elise, Carron, Jérôme, Cavazzuti, Elisabetta, Fiorini, Mauro, Khosropanah, Pourya, Martin, Sylvain, Perry, James, Pinsard, Frederic, Pradines, Alice, Rigano, Manuela, Roelfsema, Peter, Schwander, Denis, Torrioli, Guido, Ullom, Joel, Vera, Isabel, Villegas, Eduardo Medinaceli, Zuchniak, Monika, Brachet, Frank, Cicero, Ugo Lo, Doriese, William, Durkin, Malcom, Fioretti, Valentina, Geoffray, Hervé, Jacques, Lionel, Kirsch, Christian, Smith, Stephen, Adams, Joseph, Gloaguen, Emilie, Hoogeveen, Ruud, van der Hulst, Paul, Kiviranta, Mikko, van der Kuur, Jan, Ledot, Aurélien, van Leeuwen, Bert-Joost, van Loon, Dennis, Lyautey, Bertrand, Parot, Yann, Sakai, Kazuhiro, van Weers, Henk, Abdoelkariem, Shariefa, Adam, Thomas, Adami, Christophe, Aicardi, Corinne, Akamatsu, Hiroki, Alonso, Pablo Eleazar Merino, Amato, Roberta, André, Jérôme, Angelinelli, Matteo, Anon-Cancela, Manuel, Anvar, Shebli, Atienza, Ricardo, Attard, Anthony, Auricchio, Natalia, Balado, Ana, Bancel, Florian, Barusso, Lorenzo Ferrari, Bernard, Vivian, Berrocal, Alicia, Blin, Sylvie, Bonino, Donata, Bonnet, François, Bonny, Patrick, Boorman, Peter, Boreux, Charles, Bounab, Ayoub, Boutelier, Martin, Boyce, Kevin, Brienza, Daniele, Bruijn, Marcel, Bulgarelli, Andrea, Calarco, Simona, Callanan, Paul, Camus, Thierry, Canourgues, Florent, Capobianco, Vito, Cardiel, Nicolas, Castellani, Florent, Cheatom, Oscar, Chervenak, James, Chiarello, Fabio, Clerc, Nicolas, Clerc, Laurent, Cobo, Beatriz, Coeur-Joly, Odile, Coleiro, Alexis, Colonges, Stéphane, Corcione, Leonardo, Coriat, Mickael, Coynel, Alexandre, Cuttaia, Francesco, D'Ai, Antonino, D'anca, Fabio, Dadina, Mauro, Daniel, Christophe, DeNigris, Natalie, Dercksen, Johannes, DiPirro, Michael, Doumayrou, Eric, Dubbeldam, Luc, Dupieux, Michel, Dupourqué, Simon, Durand, Jean Louis, Eckert, Dominique, Eiriz, Valvanera, Ercolani, Eric, Etcheverry, Christophe, Finkbeiner, Fred, Fiocchi, Mariateresa, Fossecave, Hervé, Franssen, Philippe, Frericks, Martin, Gabici, Stefano, Gant, Florent, Gao, Jian-Rong, Gastaldello, Fabio, Genolet, Ludovic, Ghizzardi, Simona, Gil, M Angeles Alcacera, Giovannini, Elisa, Godet, Olivier, Gomez-Elvira, Javier, Gonzalez, Manuel, Gonzalez, Raoul, Gottardi, Luciano, Granat, Dolorès, Gros, Michel, Guignard, Nicolas, Hieltjes, Paul, Hurtado, Adolfo Jesus, Irwin, Kent, Jacquey, Christian, Janiuk, Agnieszka, Jaubert, Jean, Jiménez, Maria, Jolly, Antoine, Jourdan, Thierry, Julien, Sabine, Kedziora, Bartosz, Korb, Andrew, Kreykenbohm, Ingo, König, Ole, Langer, Mathieu, Laudet, Philippe, Laurent, Philippe, Laurenza, Monica, Lesrel, Jean, Ligori, Sebastiano, Lorenz, Maximilian, Luminari, Alfredo, Maffei, Bruno, Maisonnave, Océane, Marelli, Lorenzo, Massonet, Didier, Maussang, Irwin, Melchor, Alejandro Gonzalo, Mer, Isabelle Le, Michalski, Lea, Millerioux, Jean-Pierre, Mineo, Teresa, Minervini, Gabriele, Molin, Alexeï, Monestes, David, Montinaro, Nicola, Mot, Baptiste, Murat, David, Nagayoshi, Kenichiro, Nazé, Yaël, Noguès, Loïc, Pailot, Damien, Panessa, Francesca, Parodi, Luigi, Petit, Pascal, Piconcelli, Enrico, Pinto, Ciro, Plaza, Jose Miguel Encinas, Poyatos, David, Prouvé, Thomas, Ptak, Andy, Puccetti, Simonetta, Puccio, Elena, Ramon, Pascale, Reina, Manuel, Rioland, Guillaume, Rodriguez, Louis, Roig, Anton, Rollet, Bertrand, Roncarelli, Mauro, Roudil, Gilles, Rudnicki, Tomasz, Sanisidro, Julien, Sciortino, Luisa, Silva, Vitor, Sordet, Michael, Soto-Aguilar, Javier, Spizzi, Pierre, Surace, Christian, Sánchez, Miguel Fernández, Taralli, Emanuele, Terrasa, Guilhem, Terrier, Régis, Todaro, Michela, Ubertini, Pietro, Uslenghi, Michela, de Vaate, Jan Geralt Bij, Vaccaro, Davide, Varisco, Salvatore, Varnière, Peggy, Vibert, Laurent, Vidriales, María, Villa, Fabrizio, Vodopivec, Boris Martin, Volpe, Angela, de Vries, Cor, Wakeham, Nicholas, Walmsley, Gavin, Wise, Michael, de Wit, Martin, Woźniak, Grzegorz
The Athena X-ray Integral Unit (X-IFU) is the high resolution X-ray spectrometer, studied since 2015 for flying in the mid-30s on the Athena space X-ray Observatory, a versatile observatory designed to address the Hot and Energetic Universe science t
Externí odkaz:
http://arxiv.org/abs/2208.14562
Autor:
Giuffrida, Roberta, Miceli, Marco, Caprioli, Damiano, Decourchelle, Anne, Vink, Jacco, Orlando, Salvatore, Bocchino, Fabrizio, Greco, Emanuele, Peres, Giovanni
The origin of cosmic rays is a pivotal open issue of high-energy astrophysics. Supernova remnants are strong candidates to be the Galactic factory of cosmic rays, their blast waves being powerful particle accelerators. However, supernova remnants can
Externí odkaz:
http://arxiv.org/abs/2208.14491
Autor:
Ferrand, Gilles, Tanikawa, Ataru, Warren, Donald C., Nagataki, Shigehiro, Safi-Harb, Samar, Decourchelle, Anne
Type Ia supernovae (SNe) are believed to be caused by the thermonuclear explosion of a white dwarf (WD), but the nature of the progenitor system(s) is still unclear. Recent theoretical and observational developments have led to renewed interest in do
Externí odkaz:
http://arxiv.org/abs/2202.04268
Autor:
Barret, Didier, Decourchelle, Anne, Fabian, Andy, Guainazzi, Matteo, Nandra, Kirpal, Smith, Randall, Herder, Jan-Willem den
The properties (temperature, density, chemical composition, velocity) of hot astrophysical plasma and the physical processes affecting them (heating/cooling, turbulence, shocks, acceleration) can be probed by high resolution X-ray spectroscopy, to be
Externí odkaz:
http://arxiv.org/abs/1912.04615
Autor:
Roberta Giuffrida, Marco Miceli, Damiano Caprioli, Anne Decourchelle, Jacco Vink, Salvatore Orlando, Fabrizio Bocchino, Emanuele Greco, Giovanni Peres
Publikováno v:
Nature Communications, Vol 13, Iss 1, Pp 1-11 (2022)
It is known that cosmic rays could be accelerated by shock waves in supernova (SN) remnants. Here, the authors show that SN 1006 remnant is an efficient source of cosmic rays, providing observational support for the quasi-parallel acceleration mechan
Externí odkaz:
https://doaj.org/article/af3e18d9cd6b4884a957d6ac7451f12d
Autor:
Li, Jiang-Tao, Ballet, Jean, Miceli, Marco, Zhou, Ping, Vink, Jacco, Chen, Yang, Acero, Fabio, Decourchelle, Anne, Bregman, Joel N.
We present ~400ks NuSTAR observations of the northeast (NE) and southwest (SW) non-thermal limbs of the Galactic SNR SN1006. We discovered three sources with X-ray emission detected at >50keV. Two of them are identified as background AGN. We extract
Externí odkaz:
http://arxiv.org/abs/1807.09622
Autor:
Barret, Didier, Trong, Thien Lam, Herder, Jan-Willem den, Piro, Luigi, Cappi, Massimo, Huovelin, Juhani, Kelley, Richard, Mas-Hesse, J. Miguel, Mitsuda, Kazuhisa, Paltani, Stéphane, Rauw, Gregor, Rozanska, Agata, Wilms, Joern, Bandler, Simon, Barbera, Marco, Barcons, Xavier, Bozzo, Enrico, Ceballos, Maria Teresa, Charles, Ivan, Costantini, Elisa, Decourchelle, Anne, Hartog, Roland den, Duband, Lionel, Duval, Jean-Marc, Fiore, Fabrizio, Gatti, Flavio, Goldwurm, Andrea, Jackson, Brian, Jonker, Peter, Kilbourne, Caroline, Macculi, Claudio, Mendez, Mariano, Molendi, Silvano, Orleanski, Piotr, Pajot, François, Pointecouteau, Etienne, Porter, Frederick, Pratt, Gabriel W., Prêle, Damien, Ravera, Laurent, Sato, Kosuke, Schaye, Joop, Shinozaki, Keisuke, Thibert, Tanguy, Valenziano, Luca, Valette, Veronique, Vink, Jacco, Webb, Natalie, Wise, Michael, Yamasaki, Noriko, Delcelier-Douchin, Françoise, Mesnager, Jean-Michel, Pontet, Bernard, Pradines, Alice, Branduardi-Raymont, Graziella, Bulbul, Esra, Dadina, Mauro, Ettori, Stefano, Finoguenov, Alexis, Fukazawa, Yasushi, Janiuk, Agnieszka, Kaastra, Jelle, Mazzotta, Pasquale, Miller, Jon, Miniutti, Giovanni, Nazé, Yaël, Nicastro, Fabrizio, Sciortino, Salvatore, Simionescu, Aurora, Torrejon, Jose Miguel, Frezouls, Benoît, Geoffray, Hervé, Peille, Philippe, Aicardi, Corinne, André, Jérôme, Clénet, Antoine, Daniel, Christophe, Etcheverry, Christophe, Gloaguen, Emilie, Hervet, Gilles, Jolly, Antoine, Ledot, Aurélien, Maussang, Irwin, Paillet, Alexis, Schmisser, Roseline, Vella, Bruno, Damery, Jean-Charles, Boyce, Kevin, DiPirro, Michael, Lotti, Simone, Schwander, Denis, Smith, Stephen, van Leeuwen, Bert-Joost, van Weers, Henk, Clerc, Nicolas, Cobo, Beatriz, Dauser, Thomas, de Plaa, Jelle, Kirsch, Christian, Cucchetti, Edoardo, Eckart, Megan, Ferrando, Philippe, Natalucci, Lorenzo
The X-ray Integral Field Unit (X-IFU) is the high resolution X-ray spectrometer of the ESA Athena X-ray observatory. Over a field of view of 5' equivalent diameter, it will deliver X-ray spectra from 0.2 to 12 keV with a spectral resolution of 2.5 eV
Externí odkaz:
http://arxiv.org/abs/1807.06092
Autor:
Barret, Didier, Trong, Thien Lam, Herder, Jan-Willem den, Piro, Luigi, Barcons, Xavier, Huovelin, Juhani, Kelley, Richard, Mas-Hesse, J. Miguel, Mitsuda, Kazuhisa, Paltani, Stéphane, Rauw, Gregor, Rożanska, Agata, Wilms, Joern, Barbera, Marco, Bozzo, Enrico, Ceballos, Maria Teresa, Charles, Ivan, Decourchelle, Anne, Hartog, Roland den, Duval, Jean-Marc, Fiore, Fabrizio, Gatti, Flavio, Goldwurm, Andrea, Jackson, Brian, Jonker, Peter, Kilbourne, Caroline, Macculi, Claudio, Mendez, Mariano, Molendi, Silvano, Orleanski, Piotr, Pajot, François, Pointecouteau, Etienne, Porter, Frederick, Pratt, Gabriel W., Prêle, Damien, Ravera, Laurent, Renotte, Etienne, Schaye, Joop, Shinozaki, Keisuke, Valenziano, Luca, Vink, Jacco, Webb, Natalie, Yamasaki, Noriko, Delcelier-Douchin, Françoise, Du, Michel Le, Mesnager, Jean-Michel, Pradines, Alice, Branduardi-Raymont, Graziella, Dadina, Mauro, Finoguenov, Alexis, Fukazawa, Yasushi, Janiuk, Agnieszka, Miller, Jon, Nazé, Yaël, Nicastro, Fabrizio, Sciortino, Salvatore, Torrejon, Jose Miguel, Geoffray, Hervé, Hernandez, Isabelle, Luno, Laure, Peille, Philippe, André, Jérôme, Daniel, Christophe, Etcheverry, Christophe, Gloaguen, Emilie, Hassin, Jérémie, Hervet, Gilles, Maussang, Irwin, Moueza, Jérôme, Paillet, Alexis, Vella, Bruno, Garrido, Gonzalo Campos, Damery, Jean-Charles, Panem, Chantal, Panh, Johan, Bandler, Simon, Biffi, Jean-Marc, Boyce, Kevin, Clénet, Antoine, DiPirro, Michael, Jamotton, Pierre, Lotti, Simone, Schwander, Denis, Smith, Stephen, van Leeuwen, Bert-Joost, van Weers, Henk, Brand, Thorsten, Cobo, Beatriz, Dauser, Thomas, de Plaa, Jelle, Cucchetti, Edoardo
Publikováno v:
Proc. SPIE. 9905, Space Telescopes and Instrumentation 2016: Ultraviolet to Gamma Ray, 99052F. (August 17, 2016)
The X-ray Integral Field Unit (X-IFU) on board the Advanced Telescope for High-ENergy Astrophysics (Athena) will provide spatially resolved high-resolution X-ray spectroscopy from 0.2 to 12 keV, with 5 arc second pixels over a field of view of 5 arc
Externí odkaz:
http://arxiv.org/abs/1608.08105