Zobrazeno 1 - 10
of 45
pro vyhledávání: '"K. S. Long"'
Autor:
F. M. Vincentelli, J. Neilsen, A. J. Tetarenko, Y. Cavecchi, N. Castro Segura, S. del Palacio, J. van den Eijnden, G. Vasilopoulos, D. Altamirano, M. Armas Padilla, C. D. Bailyn, T. Belloni, D. J. K. Buisson, V. A. Cúneo, N. Degenaar, C. Knigge, K. S. Long, F. Jiménez-Ibarra, J. Milburn, T. Muñoz Darias, M. Özbey Arabacı, R. Remillard, T. Russell
Accretion disks around compact objects are expected to enter an unstable phase at high luminosity. One instability may occur when the radiation pressure generated by accretion modifies the disk viscosity, resulting in the cyclic depletion and refilli
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::0cbde99a5ba53c3a1e4148acf451f3f5
https://eprints.soton.ac.uk/476105/
https://eprints.soton.ac.uk/476105/
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
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 511:5385-5395
WZ Sge is the prototype of highly evolved, low-accretion rate dwarf novae (DNe). During the decline from eruptions, its light curve displays a ‘dip’ followed by ≃10 ‘echo outbursts’. The standard disc instability model does not account for
The optical emission line spectra of X-ray binaries (XRBs) are thought to be produced in an irradiated atmosphere, possibly the base of a wind, located above the outer accretion disc. However, the physical nature of - and physical conditions in - the
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::995a25f323232a0ba8a4659f4a420237
Autor:
K Inight, B T Gänsicke, D Blondel, D Boyd, R P Ashley, C Knigge, K S Long, T R Marsh, J McCleery, S Scaringi, D Steeghs, J R Thorstensen, T Vanmunster, P J Wheatley
Publikováno v:
Monthly Notices of the Royal Astronomical Society, 2021, Vol.510(3), pp.3605-3621 [Peer Reviewed Journal]
Despite being bright ($V=12$) and nearby ($d=212$ pc) ASAS J071404+7004.3 has only recently been identified as a nova-like cataclysmic variable. We present time-resolved optical spectroscopy obtained at the Isaac Newton Telescope together with $\text
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::3c90c58f0b0996a1bf8e97d0683e5389
http://arxiv.org/abs/2109.14514
http://arxiv.org/abs/2109.14514
Akademický článek
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Publikováno v:
American journal of hospital pharmacy. 50(6)
An evaluation of ondansetron use in oncology patients in three hospitals is described. Criteria for the use of ondansetron were developed and approved by each hospital's pharmacy and therapeutics committee or medical staff executive committee. Ondans
Publikováno v:
International Astronomical Union Colloquium. 194:251-251
We present initial results of a survey of the FUV spectra of disk-accreting cataclysmic variables obtained with the Far Ultraviolet Spectroscopic Explorer (FUSE).FUSE covers the 905 - 1188 Å range at spectral resolutions ≃0.1 Å. To date, FUSE has
Akademický článek
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