Zobrazeno 1 - 10
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pro vyhledávání: '"Arias, María A."'
Autor:
Petruk, Oleh, Kuzyo, Taras, Patrii, Mariana, Chomiuk, Laura, Arias, Maria, Miceli, Marco, Orlando, Salvatore, Bocchino, Fabrizio
By using surface brightness maps of Tycho's supernova remnant (SNR) in radio and X-rays, along with the properties of thermal and synchrotron emission, we have derived the post-shock density and magnetic field strength distributions over the projecti
Externí odkaz:
http://arxiv.org/abs/2407.10929
Autor:
Arias, Maria, Zhou, Ping, Chiotellis, Alexandros, De Breuck, Carlos, Domcek, Vladimir, Boumis, Panos, Vink, Jacco, Derlopa, Sophia, Akras, Stavros
Supernova remnants (SNRs) are profoundly affected by their ambient medium. We present carbon monoxide (CO) observations around two mixed morphology SNRs, VRO 42.05.01 and G 350.0-2.0, that look remarkably similar in continuum radio emission, showing
Externí odkaz:
http://arxiv.org/abs/2402.10763
Autor:
Schoedel, Rainer, Longmore, Steve, Henshaw, Jonny, Ginsburg, Adam, Bally, John, Feldmeier, Anja, Hosek, Matt, Lara, Francisco Nogueras, Ciurlo, Anna, Chevance, Mélanie, Kruijssen, J. M. Diederik, Klessen, Ralf, Ponti, Gabriele, Amaro-Seoane, Pau, Anastasopoulou, Konstantina, Anderson, Jay, Arias, Maria, Barnes, Ashley T., Battersby, Cara, Bono, Giuseppe, Ferres, Lucía Bravo, Bryant, Aaron, Gonzáalez, Miguel Cano, Cassisi, Santi, Chaves-Velasquez, Leonardo, Conte, Francesco, Ramos, Rodrigo Contreras, Cotera, Angela, Crowe, Samuel, di Teodoro, Enrico, Do, Tuan, Eisenhauer, Frank, Enokiya, Rei, Fedriani, Rubén, Friske, Jennifer K. S., Gadotti, Dimitri, Gallart, Carme, Calvente, Teresa Gallego, Cano, Eulalia Gallego, Fuentes, Pablo García, Marín, Macarena García, Gardini, Angela, Gautam, Abhimat K., Ghez, Andrea, Gillessen, Stefan, Gouda, Naoteru, Gualandris, Alessia, Guarcello, Mario Giuseppe, Gutermuth, Robert, Haggard, Daryl, Hankins, Matthew, Hu, Yue, Kano, Ryohei, Kauffmann, Jens, Lau, Ryan, Lazarian, Alexandre, Libralato, Mattia, Lu, Anan, Lu, Xing, Lu, Jessica R., Luetzgendorf, Nora, Magorrian, John, Mandel, Shifra, Markoff, Sera, Arranz, Álvaro Martínez, Mastrobuono-Battisti, Alessandra, Melamed, Maria, Mills, Elisabeth, Mori, Kaya, Morris, Mark, Murchikova, Elena, Nagata, Tetsuya, Najarro, Francisco, Nandakumar, Govind, Nataf, David, Neumayer, Nadine, Nishiyama, Shogo, Nobukawa, Masayoshi, Paré, Dylan M, Peissker, Florian, Petkova, Maya, Pillai, Thushara G. S., Román, Mike Rich Carlos, Rugel, Michael, Ryde, Nils, Sabha, Nadeen, Bermúdez, Joel Sánchez, Sánchez-Monge, Álvaro, Schultheis, Mathias, Shao, Lijing, Shinnaga, Hiroko, Simpson, Janet, Takekawa, Shunya, Tan, Jonathan C., Thorsbro, Brian, Torne, Pablo, Tress, Robin Goppala, Uchiyam, Hideki, Valenti, Elena, van der Marel, Roeland, Verberne, Sill, Vermot, Pierre, von Fellenberg, Sebastiano, Walker, Daniel, Witzel, Gunther, Xu, Siyao, Yano, Taihei, Yusef-Zadeh, Farhad, Zajaček, Michal, Zoccali, Manuela
The inner hundred parsecs of the Milky Way hosts the nearest supermassive black hole, largest reservoir of dense gas, greatest stellar density, hundreds of massive main and post main sequence stars, and the highest volume density of supernovae in the
Externí odkaz:
http://arxiv.org/abs/2310.11912
Publikováno v:
Galaxies, 11, 72 (2023)
The B[e] phenomenon is manifested by a heterogeneous group of stars surrounded by gaseous and dusty circumstellar envelopes with similar physical conditions. Among these stars, the FS CMa-type objects are suspected to be binary systems, which could b
Externí odkaz:
http://arxiv.org/abs/2306.16536
Autor:
Kraus, Michaela, Kourniotis, Michalis, Arias, Maria Laura, Torres, Andrea F., Nickeler, Dieter H.
Publikováno v:
Galaxies, 11, 76 (2023)
Massive stars expel large amounts of mass during their late evolutionary phases. We aim to unveil the physical conditions within the warm molecular environments of B[e] supergiants (B[e]SGs) and yellow hypergiants (YHGs), which are known to be embedd
Externí odkaz:
http://arxiv.org/abs/2306.10911
Autor:
Gregory, Wilson, Hogg, David W., Blum-Smith, Ben, Arias, Maria Teresa, Wong, Kaze W. K., Villar, Soledad
Convolutional neural networks and their ilk have been very successful for many learning tasks involving images. These methods assume that the input is a scalar image representing the intensity in each pixel, possibly in multiple channels for color im
Externí odkaz:
http://arxiv.org/abs/2305.12585
Multivalued projections are applied to the study of weighted least squares solutions of linear relations equations (or inclusions) and some of its applications. To this end a matrix representation of multivalued projections with respect to the closur
Externí odkaz:
http://arxiv.org/abs/2301.12997
A linear relation $E$ acting on a Hilbert space is idempotent if $E^2=E.$ A triplet of subspaces is needed to characterize a given idempotent: $(\mathrm{ran} \, E, \mathrm{ran}(I-E), \mathrm{dom}\, E),$ or equivalently, $(\mathrm{ker}(I-E), \mathrm{k
Externí odkaz:
http://arxiv.org/abs/2204.03581
Autor:
Zhou, Ping, Zhang, Gao-Yuan, Zhou, Xin, Arias, Maria, Koo, Bon-Chul, Vink, Jacco, Zhang, Zhi-Yu, Sun, Lei, Du, Fu-Jun, Zhu, Hui, Chen, Yang, Bovino, Stefano, Lee, Yong-Hyun
Galactic supernova remnants (SNRs) and their environments provide the nearest laboratories to study SN feedback. We performed molecular observations toward SNR W49B, the most luminous Galactic SNR in the X-ray band, aiming to explore signs of multipl
Externí odkaz:
http://arxiv.org/abs/2203.13111
Autor:
Fuentes, Fernanda, Contreras, Maria Jose, Arroyo-Salvo, Camila, Cabrera P, Paulina, Silva, Mauricio, Merino, Osvaldo, Arias, Maria Elena, Felmer, Ricardo
Publikováno v:
In Theriogenology 15 September 2024 226:29-38
