Zobrazeno 1 - 6
of 6
pro vyhledávání: '"Pires, Adriana Mancini"'
Autor:
Pires, Adriana Mancini, Motch, Christian, Schwope, Axel, Traulsen, Iris, Ballet, Jean, Chakraborty, Sudip, Homan, David, Kurpas, Jan, Gomez-Moran, Ada Nebot, Pineau, Francois-Xavier, Tranin, Hugo, Webb, Natalie
The discovery of radio-quiet, X-ray thermally emitting isolated neutron stars (XINSs) in the ROSAT All-Sky Survey revealed a previously overlooked component of the neutron star population. Advancements in X-ray instrumentation and the availability of
Externí odkaz:
http://arxiv.org/abs/2412.03870
We report the initial results of deep eROSITA monitoring of the "magnificent seven" isolated neutron stars (INSs). Thanks to a combination of high count statistics and good energy resolution, the eROSITA datasets unveil the increasingly complex energ
Externí odkaz:
http://arxiv.org/abs/2202.06793
Autor:
Pires, Adriana Mancini
The observational manifestation of a neutron star is strongly connected with the properties of its magnetic field. During the star's lifetime, the field strength and its changes dominate the thermo-rotational evolution and the source phenomenology ac
Externí odkaz:
http://arxiv.org/abs/1711.05045
Autor:
Pires, Adriana Mancini
Since the discovery of the first radio pulsar fifty years ago, the population of neutron stars in our Galaxy has grown to over 2,600. A handful of these sources, exclusively seen in X-rays, show properties that are not observed in normal pulsars. Des
Externí odkaz:
http://arxiv.org/abs/1711.05038
Autor:
Pires, Adriana Mancini
The new results of our observing campaign targeting the isolated neutron star 2XMM J104608.7-594306 in the Carina Nebula are used to understand how peculiar groups of isolated neutron stars relate to each other, as well as to the bulk of the normal r
Externí odkaz:
http://arxiv.org/abs/1206.3494
Autor:
Pires, Adriana Mancini, Motch, Christian, Turolla, Roberto, Schwope, Axel, Pilia, Maura, Treves, Aldo, Popov, Sergei B., Janot-Pacheco, Eduardo
Publikováno v:
Astronomy & Astrophysics, Volume 544, id.A17 (2012)
While fewer in number than the dominant rotation-powered radio pulsar population, peculiar classes of isolated neutron stars (INSs) -- which include magnetars, the ROSAT-discovered "Magnificent Seven" (M7), rotating radio transients (RRATs), and cent
Externí odkaz:
http://arxiv.org/abs/1205.0427