Zobrazeno 1 - 3
of 3
pro vyhledávání: '"J V Hernandez Santisteban"'
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]
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
https://doi.org/10.1038/s41586-021-04324-2
Autor:
N Castro Segura, C Knigge, J A Acosta-Pulido, D Altamirano, S del Palacio, J V Hernandez Santisteban, M Pahari, P Rodriguez-Gil, C Belardi, D A H Buckley, M R Burleigh, M Childress, R P Fender, D M Hewitt, D J James, R B Kuhn, N P M Kuin, J Pepper, A A Ponomareva, M L Pretorius, J E Rodríguez, K G Stassun, D R A Williams, P A Woudt
Publikováno v:
Castro Segura, N, Knigge, C, Acosta-Pulido, J A, Altamirano, D, del Palacio, S, Hernandez Santisteban, J V, Pahari, M, Rodriguez-Gil, P, Belardi, C, Buckley, D A H, Burleigh, M R, Childress, M, Fender, R P, Hewitt, D M, James, D J, Kuhn, R B, Kuin, N P M, Pepper, J, Ponomareva, A A, Pretorius, M L, Rodríguez, J E, Stassun, K G, Williams, D R A & Woudt, P A 2021, ' Bow shocks, nova shells, disc winds and tilted discs: the nova-like V341 Ara has it all ', Monthly Notices of the Royal Astronomical Society, vol. 501, no. 2, pp. 1951-1969 . https://doi.org/10.1093/mnras/staa2516
CONICET Digital (CONICET)
Consejo Nacional de Investigaciones Científicas y Técnicas
instacron:CONICET
CONICET Digital (CONICET)
Consejo Nacional de Investigaciones Científicas y Técnicas
instacron:CONICET
V341 Ara was recently recognised as one of the closest (d ~ 150 pc) and brightest (V~ 10) nova-like cataclysmic variables. This unique system is surrounded by a bright emission nebula, likely to be the remnant of a recent nova eruption. Embedded with
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::141bf331554df5104d38e5e50d5675eb
https://eprints.soton.ac.uk/443666/
https://eprints.soton.ac.uk/443666/
Autor:
Castro Segura, N., Knigge, C., Long, K. S., Altamirano, D., Armas Padilla, M., Bailyn, C., Buckley, D. A. H., Buisson, D. J. K., Casares, J., Charles, P., Combi, J. A., Cúneo, V. A., Degenaar, N. D., del Palacio, S., Díaz Trigo, M., Fender, R., Gandhi, P., Georganti, M., Gutiérrez, C., Hernandez Santisteban, J. V.
Publikováno v:
Nature; 3/3/2022, Vol. 603 Issue 7899, p52-57, 6p