Zobrazeno 1 - 10
of 11 227
pro vyhledávání: '"A Anitra"'
Autor:
Anitra, A., Miceli, C., Di Salvo, T., Iaria, R., Degenaar, N., Miller, M. Jon, Barra, F., Leone, W., Burderi, L.
We propose a novel approach for determining the orbital inclination of low-mass X-ray binary systems by modelling the H$\alpha$ and H$\beta$ line profiles emitted by the accretion disc, with a Newtonian version of diskline. We applied the model to tw
Externí odkaz:
http://arxiv.org/abs/2409.11988
Autor:
Paulson, Susan
Publikováno v:
Environment and Society, 2021 Jan 01. 12, 257-259.
Externí odkaz:
https://www.jstor.org/stable/27204971
Autor:
Iaria, R., Di Salvo, T., Anitra, A., Miceli, C., Leone, W., Maraventano, C., Barra, F., Riggio, A., Sanna, A., Manca, A., Burderi, L.
Publikováno v:
A&A 686, A216 (2024)
XTE J1710-281 is a transient eclipsing binary system with a period close to 3.28 hours, hosting a neutron star. The average eclipse duration is 420 seconds, and eclipse arrival times reported in the literature span from 1999 to 2017. A previous analy
Externí odkaz:
http://arxiv.org/abs/2404.11203
Autor:
Bajmócy Zoltán
Publikováno v:
Tér és Társadalom, Vol 35, Iss 1 (2021)
Externí odkaz:
https://doaj.org/article/92048398777645e3b0eb6a29af98b617
Autor:
Iaria, R., Di Salvo, T., Anitra, A., Miceli, C., Barra, F., Leone, W., Burderi, L., Sanna, A., Riggio, A.
X 1822-371 is an eclipsing binary system with a period close to 5.57 hr and an orbital period derivative $\dot{P}_{\rm orb}$ of 1.42(3)$\times 10^{-10}$ s s$^{-1}$. The extremely high value of its $\dot{P}_{\rm orb}$ is compatible with a super-Edding
Externí odkaz:
http://arxiv.org/abs/2401.03698
Autor:
Alraouf, Ali A.
Publikováno v:
Traditional Dwellings and Settlements Review, 2018 Apr 01. 29(2), 92-94.
Externí odkaz:
https://www.jstor.org/stable/26877330
Autor:
Anitra, A., Sanchez, D. Mata, Munoz-Darias, T., Di Salvo, T., Iaria, R., Miceli, C., Padilla, M. Armas, Casares, J., Corral-Santana, J. M.
Swift J1357.2-0933 is a transient low-mass X-ray binary hosting a stellar-mass black hole. The source exhibits optical dips and very broad emission lines during both outburst and quiescence, which are thought to be the result of a high orbital inclin
Externí odkaz:
http://arxiv.org/abs/2310.12636
Autor:
Fabiani, Sergio, Capitanio, Fiamma, Iaria, Rosario, Poutanen, Juri, Gnarini, Andrea, Ursini, Francesco, Farinelli, Ruben, Bobrikova, Anna, Steiner, James F., Svoboda, Jiri, Anitra, Alessio, Baglio, Maria C., Carotenuto, Francesco, Del Santo, Melania, Ferrigno, Carlo, Lewis, Fraser, Russell, David M., Russell, Thomas D., Eijnden, Jakob van den, Cocchi, Massimo, Di Marco, Alessandro, La Monaca, Fabio, Liu, Kuan, Rankin, John, Weisskopf, Martin C., Xie, Fei, Bianchi, Stefano, Burderi, Luciano, Di Salvo, Tiziana, Egron, Elise, Illiano, Giulia, Kaaret, Philip, Matt, Giorgio, Mikušincová, Romana, Muleri, Fabio, Papitto, Alessandro, Agudo, Iván, Antonelli, Lucio A., Bachetti, Matteo, Baldini, Luca, Baumgartner, Wayne H., Bellazzini, Ronaldo, Bongiorno, Stephen D., Bonino, Raffaella, Brez, Alessandro, Bucciantini, Niccolò, Castellano, Simone, Cavazzuti, Elisabetta, Chen, Chien-Ting, Ciprini, Stefano, Costa, Enrico, De Rosa, Alessandra, Del Monte, Ettore, Di Gesu, Laura, Di Lalla, Niccolò, Donnarumma, Immacolata, Doroshenko, Victor, Dovčiak, Michal, Ehlert, Steven R., Enoto, Teruaki, Evangelista, Yuri, Ferrazzoli, Riccardo, Garcia, Javier A., Gunji, Shuichi, Hayashida, Kiyoshi, Heyl, Jeremy, Iwakiri, Wataru, Jorstad, Svetlana G., Karas, Vladimir, Kislat, Fabian, Kitaguchi, Takao, Kolodziejczak, Jeffery J., Krawczynski, Henric, Latronico, Luca, Liodakis, Ioannis, Maldera, Simone, Manfreda, Alberto, Marin, Frédéric, Marinucci, Andrea, Marscher, Alan P., Marshall, Herman L., Massaro, Francesco, Mitsuishi, Ikuyuki, Mizuno, Tsunefumi, Negro, Michela, Ng, Chi-Yung, O'Dell, Stephen L., Omodei, Nicola, Oppedisano, Chiara, Pavlov, George G., Peirson, Abel L., Perri, Matteo, Pesce-Rollins, Melissa, Petrucci, Pierre-Olivier, Pilia, Maura, Possenti, Andrea, Puccetti, Simonetta, Ramsey, Brian D., Ratheesh, Ajay, Roberts, Oliver J., Romani, Roger W., Sgrò, Carmelo, Slane, Patrick, Soffitta, Paolo, Spandre, Gloria, Swartz, Douglas A., Tamagawa, Toru, Tavecchio, Fabrizio, Taverna, Roberto, Tawara, Yuzuru, Tennant, Allyn F., Thomas, Nicholas E., Tombesi, Francesco, Trois, Alessio, Tsygankov, Sergey S., Turolla, Roberto, Vink, Jacco, Wu, Kinwah, Zane, Silvia
We report on the coordinated observations of the neutron star low-mass X-ray binary (NS-LMXB) \gx in X-rays (IXPE, NICER, Nustar and INTEGRAL), optical (REM and LCO), near-infrared (REM), mid-infrared (VLT VISIR), and radio (ATCA). This Z-source was
Externí odkaz:
http://arxiv.org/abs/2310.06788
Autor:
Price, R. Jordan1 (AUTHOR), Davik, Jahn2 (AUTHOR), Fernandéz Fernandéz, Felicidad3 (AUTHOR), Bates, Helen J.1 (AUTHOR), Lynn, Samantha3 (AUTHOR), Nellist, Charlotte F.1 (AUTHOR), Buti, Matteo4 (AUTHOR), Røen, Dag5 (AUTHOR), Šurbanovski, Nada3 (AUTHOR), Alsheikh, Muath5 (AUTHOR), Harrison, Richard J.1 (AUTHOR), Sargent, Daniel James3 (AUTHOR) dan.sargent@niab.com
Publikováno v:
PLoS ONE. 5/16/2023, Vol. 17 Issue 5, p1-17. 17p.