Zobrazeno 1 - 10
of 357
pro vyhledávání: '"C, Knigge"'
Autor:
A. W. Shaw, D. L. Kaplan, P. Gandhi, T. J. Maccarone, E. S. Borowski, C. T. Britt, D. A. H. Buckley, K. B. Burdge, P. A. Charles, V. S. Dhillon, R. G. French, C. O. Heinke, R. I. Hynes, C. Knigge, S. P. Littlefair, Devraj Pawar, R. M. Plotkin, M. E. Ressler, P. Santos-Sanz, T. Shahbaz, G. R. Sivakoff, A. L. Stevens
Publikováno v:
The Astronomical Journal, Vol 169, Iss 1, p 21 (2024)
JWST, despite not being designed to observe astrophysical phenomena that vary on rapid timescales, can be an unparalleled tool for such studies. If timing systematics can be controlled, JWST will be able to open up the subsecond infrared timescale re
Externí odkaz:
https://doaj.org/article/f8dde5a8ec1b4aca9ca4d9b7e1e00493
Autor:
A. Hellsten, K. Ketelsen, M. Sühring, M. Auvinen, B. Maronga, C. Knigge, F. Barmpas, G. Tsegas, N. Moussiopoulos, S. Raasch
Publikováno v:
Geoscientific Model Development, Vol 14, Pp 3185-3214 (2021)
Large-eddy simulation (LES) provides a physically sound approach to study complex turbulent processes within the atmospheric boundary layer including urban boundary layer flows. However, such flow problems often involve a large separation of turbulen
Externí odkaz:
https://doaj.org/article/6d6329ec44ba4557bf4fd19d9f5bd030
Autor:
B. Maronga, S. Banzhaf, C. Burmeister, T. Esch, R. Forkel, D. Fröhlich, V. Fuka, K. F. Gehrke, J. Geletič, S. Giersch, T. Gronemeier, G. Groß, W. Heldens, A. Hellsten, F. Hoffmann, A. Inagaki, E. Kadasch, F. Kanani-Sühring, K. Ketelsen, B. A. Khan, C. Knigge, H. Knoop, P. Krč, M. Kurppa, H. Maamari, A. Matzarakis, M. Mauder, M. Pallasch, D. Pavlik, J. Pfafferott, J. Resler, S. Rissmann, E. Russo, M. Salim, M. Schrempf, J. Schwenkel, G. Seckmeyer, S. Schubert, M. Sühring, R. von Tils, L. Vollmer, S. Ward, B. Witha, H. Wurps, J. Zeidler, S. Raasch
Publikováno v:
Geoscientific Model Development, Vol 13, Pp 1335-1372 (2020)
In this paper, we describe the PALM model system 6.0. PALM (formerly an abbreviation for Parallelized Large-eddy Simulation Model and now an independent name) is a Fortran-based code and has been applied for studying a variety of atmospheric and ocea
Externí odkaz:
https://doaj.org/article/66dc6e54ee094e87b6d1361bba4d40e5
Publikováno v:
Monthly Notices of the Royal Astronomical Society, 2022, Vol.516(1), pp.1183-1192 [Peer Reviewed Journal]
Binaries with a white dwarf primary and a main sequence secondary can be used to test our understanding of both single and binary star evolution. A small fraction of such systems experienced a common-envelope phase from which they emerged with a rela
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::21adbdc273dd4f201596b44f42721ea5
https://doi.org/10.1093/mnras/stac2197
https://doi.org/10.1093/mnras/stac2197
Akademický článek
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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
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
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::af57749a58dfe9fbe024a3c8380ee7ae
https://doi.org/10.1093/mnras/stac116
https://doi.org/10.1093/mnras/stac116
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/
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
Akademický článek
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