Zobrazeno 1 - 2
of 2
pro vyhledávání: '"general [Ray burst]"'
Autor:
M. H. Wieringa, Luigi Piro, O. D. Fox, Bing Zhang, Andrea Tiengo, T. Sakamoto, Roberto Ricci, Geoffrey Ryan, Nathaniel R. Butler, H. van Eerten, H.G. Khandrika, Eleonora Troja, Andrea Rossi, S. B. Cenko, G. Novara
Publikováno v:
Monthly Notices of the Royal Astronomical Society
Piro, L, Zhang, B, Troja, E, Ryan, G, Van Eerten, H, Ricci, R, Wieringa, M H, Tiengo, A, Butler, N, Cenko, S B, Fox, O D, Khandrika, H G, Novara, G & Sakamoto, T 2019, ' A long-lived neutron star merger remnant in GW170817 : constraints and clues from X-ray observations ', Monthly Notices of the Royal Astronomical Society, vol. 483, no. 2, pp. 1912-1921 . https://doi.org/10.1093/mnras/sty3047
Piro, L, Zhang, B, Troja, E, Ryan, G, Van Eerten, H, Ricci, R, Wieringa, M H, Tiengo, A, Butler, N, Cenko, S B, Fox, O D, Khandrika, H G, Novara, G & Sakamoto, T 2019, ' A long-lived neutron star merger remnant in GW170817 : constraints and clues from X-ray observations ', Monthly Notices of the Royal Astronomical Society, vol. 483, no. 2, pp. 1912-1921 . https://doi.org/10.1093/mnras/sty3047
Multi-messenger observations of GW170817 have not conclusively established whether the merger remnant is a black hole (BH) or a neutron star (NS). We show that a long-lived magnetized NS with a poloidal field $B\approx 10^{12}$G is fully consistent w
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::8083fc40e985893a3509c27864ebd1fc
https://doi.org/10.1093/mnras/sty3047
https://doi.org/10.1093/mnras/sty3047
Publikováno v:
Obergaulinger, M., Aloy, M. A. and Müller, E. (2010): Local simulations of the magnetized Kelvin-Helmholtz instability in neutron-star mergers, Astronomy and Astrophysics, núm. 515, vol. 5, art. no. 13386
RODERIC. Repositorio Institucional de la Universitat de Valéncia
instname
RODERIC. Repositorio Institucional de la Universitat de Valéncia
instname
Context. Global MHD simulations show Kelvin-Helmholtz (KH) instabilities at the contact surface of two merging neutron stars. That region has been identified as the site of efficient amplification of magnetic fields. However, these global simulations
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::e0cb96184d03fe3d6a836103bae24b34
https://doi.org/10.1051/0004-6361/200913386
https://doi.org/10.1051/0004-6361/200913386
