Zobrazeno 1 - 8
of 8
pro vyhledávání: '"Stecchini, Paulo E."'
In this study we revisit public data on the supersoft X-ray source CAL 83 in the Large Magellanic Cloud. A significant part of our analysis is focused on XMM-Newton X-ray observations, in which updated data reduction procedures and quality assessment
Externí odkaz:
http://arxiv.org/abs/2304.06804
Autor:
de Lima, Rafael C. R., Pereira, Jonas P., Coelho, Jaziel G., Nunes, Rafael C., Stecchini, Paulo E. F., Castro, Manuel, Gomes, Pierre, da Silva, Rodrigo R., Rodrigues, Claudia V., de Araujo, José C. N., Bejger, Michał, Haensel, Paweł, Zdunik, J. Leszek
3XMM J185246.6+003317 is a transient magnetar located in the vicinity of the supernova remnant Kes\,79. So far, observations have only set upper limits to its surface magnetic field and spindown, and there is no estimate for its mass and radius. Usin
Externí odkaz:
http://arxiv.org/abs/2210.06648
Autor:
de Lima, Rafael C.R., Pereira, Jonas P., Coelho, Jaziel G., Nunes, Rafael C., Stecchini, Paulo E., Castro, Manuel, Gomes, Pierre, da Silva, Rodrigo R., Rodrigues, Claudia V., de Araujo, José C.N., Bejger, Michał, Haensel, Paweł, Zdunik, J. Leszek
Publikováno v:
In Journal of High Energy Astrophysics June 2024 42:52-62
Autor:
Belloni, Diogo, Rodrigues, Claudia V., Schreiber, Matthias R., Castro, Manuel, Costa, Joaquim E. R., Hayashi, Takayuki, Lima, Isabel J., Luna, Gerardo J. M., Martins, Murilo, Oliveira, Alexandre S., Parsons, Steven G., Silva, Karleyne M. G., Stecchini, Paulo E., Stuchi, Teresa J., Zorotovic, Monica
We present an analysis of mock X-ray spectra and light curves of magnetic cataclysmic variables using an upgraded version of the 3D CYCLOPS code. This 3D representation of the accretion flow allows us to properly model total and partial occultation o
Externí odkaz:
http://arxiv.org/abs/2107.10861
1E 1740.7-2942 is one of the strongest hard X-ray emitters in the Galactic Centre region, believed to be a black hole in a high-mass X-ray binary system. Although extensively studied in X-rays, many aspects about the underlying nature of the system a
Externí odkaz:
http://arxiv.org/abs/2002.02951
Autor:
de Lima, Rafael C. R., Pereira, Jonas P., Coelho, Jaziel G., Nunes, Rafael C., Stecchini, Paulo E. F., Castro, Manuel, Gomes, Pierre, da Silva, Rodrigo R., Rodrigues, Claudia V., de Araujo, José C. N., Bejger, Michał, Haensel, Paweł, Zdunik, J. Leszek
3XMM J185246.6+003317 is a slowly rotating soft-gamma repeater (neutron star) in the vicinity of the supernova remnant Kes\,79. So far, observations have only set upper limits to its surface magnetic field and spindown, and there is no estimate for i
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::ac7bf84614736ab3be24a4056395f04c
Autor:
Silva, Rodrigo R., de Lima, Rafael C. R., Coelho, Jaziel G., Stecchini, Paulo E., de Liz, Caroline M., de Araujo, José C. N.
Publikováno v:
Galaxies (2075-4434); Feb2023, Vol. 11 Issue 1, p18, 10p
Publikováno v:
Monthly Notices of the Royal Astronomical Society; Apr2020, Vol. 493 Issue 2, p2694-2705, 12p