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A persistent ultraviolet outflow from an accreting neutron star binary transient

Autor: N. Castro Segura, C. Knigge, K. S. Long, D. Altamirano, M. Armas Padilla, C. Bailyn, D. A. H. Buckley, D. J. K. Buisson, J. Casares, P. Charles, J. A. Combi, V. A. Cúneo, N. D. Degenaar, S. del Palacio, M. Díaz Trigo, R. Fender, P. Gandhi, M. Georganti, C. Gutiérrez, J. V. Hernandez Santisteban, F. Jiménez-Ibarra, J. Matthews, M. Méndez, M. Middleton, T. Muñoz-Darias, M. Özbey Arabacı, M. Pahari, L. Rhodes, T. D. Russell, S. Scaringi, J. van den Eijnden, G. Vasilopoulos, F. M. Vincentelli, P. Wiseman

Publikováno v: Nature, 603(7899), 52-57. Nature Publishing Group
Nature, 603, 52-57. Nature Publishing Group
Nature, 2022, Vol.603(7899), pp.52-57 [Peer Reviewed Journal]

All disc-accreting astrophysical objects produce powerful outflows. In binaries containing neutron stars (NS) or black holes, accretion often takes place during violent outbursts. The main disc wind signatures during these eruptions are blue-shifted

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::b4bf6b5079f8fee2065ef4061ecac4d2
https://doi.org/10.1038/s41586-021-04324-2

Evidence for non-thermal X-ray emission from the double WR colliding-wind binary Apep

Autor: S. del Palacio, F. García, M. De Becker, D. Altamirano, V. Bosch-Ramon, P. Benaglia, B. Marcote, G. E. Romero

Context: Massive colliding-wind binaries (CWBs) can be non-thermal sources. The emission produced in their wind-collision region (WCR) encodes information of both the shocks properties and the relativistic electrons accelerated in them. The recently

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::6c1b2b753e7285d94b43780f616214ea

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The non-thermal emission from the colliding-wind binary Apep

Autor: S. del Palacio, P. Benaglia, M. De Becker, V. Bosch-Ramon, G. E. Romero

Publikováno v: Digital.CSIC. Repositorio Institucional del CSIC
instname
Dipòsit Digital de la UB
Universidad de Barcelona

The recently discovered massive binary system Apep is the most powerful synchrotron emitter among the known Galactic colliding-wind binaries. This makes this particular system of great interest to investigate stellar winds and the non-thermal process

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::010d370767361e00accf7cc76eb9f517
http://arxiv.org/abs/2111.07442