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of 12
pro vyhledávání: '"F. R. N. Chambers"'
Publikováno v:
Monthly Notices of the Royal Astronomical Society
Monthly Notices of the Royal Astronomical Society, 499(4), 4698-4715. Oxford University Press
Monthly Notices of the Royal Astronomical Society 499(2020)4, 4
UPCommons. Portal del coneixement obert de la UPC
Universitat Politècnica de Catalunya (UPC)
Monthly Notices of the Royal Astronomical Society, 499(4), 4698-4715. Oxford University Press
Monthly Notices of the Royal Astronomical Society 499(2020)4, 4
UPCommons. Portal del coneixement obert de la UPC
Universitat Politècnica de Catalunya (UPC)
The Cassini and Juno probes have revealed large coherent cyclonic vortices in the polar regions of Saturn and Jupiter, a dramatic contrast from the east-west banded jet structure seen at lower latitudes. Debate has centered on whether the jets are sh
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::d37d5e738396724fc79018090a9af0c8
https://doi.org/10.1093/mnras/staa2962
https://doi.org/10.1093/mnras/staa2962
Publikováno v:
Monthly Notices of the Royal Astronomical Society
Monthly Notices of the Royal Astronomical Society, 496(2), 2098-2106. Oxford University Press
Monthly Notices of the Royal Astronomical Society, 496(2), 2098-2106. Oxford University Press
Waves in thin fluid layers are important in various stellar and planetary problems. Due to rapid rotation such systems will become oblate, with a latitudinal variation in the gravitational acceleration across the surface of the object. In the case of
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::4a028baf02bf27b6738340e321c7be7b
https://dare.uva.nl/personal/pure/en/publications/waves-in-thin-oceans-on-oblate-neutron-stars(ad947f79-0fcc-44af-93bd-1631d7bea0d3).html
https://dare.uva.nl/personal/pure/en/publications/waves-in-thin-oceans-on-oblate-neutron-stars(ad947f79-0fcc-44af-93bd-1631d7bea0d3).html
Autor:
F. R. N. Chambers, Anna L. Watts
Publikováno v:
Monthly Notices of the Royal Astronomical Society, 491(4), 6032-6044. Oxford University Press
Monthly Notices of the Royal Astronomical Society
Monthly Notices of the Royal Astronomical Society
Accreting neutron stars (NS) can exhibit high frequency modulations in their lightcurves during thermonuclear X-ray bursts, known as burst oscillations. These frequencies can be offset from the NS spin frequency by several Hz (where known independent
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::83e0adddacb0e2bdf3673ede985c51df
https://hdl.handle.net/11245.1/df7bba7d-9a81-4f16-9e22-57a3a0507612
https://hdl.handle.net/11245.1/df7bba7d-9a81-4f16-9e22-57a3a0507612
Publikováno v:
Monthly Notices of the Royal Astronomical Society
Monthly Notices of the Royal Astronomical Society, 505(4), 5530-5542. Oxford University Press
Monthly Notices of the Royal Astronomical Society, 505(4), 5530-5542. Oxford University Press
Hotspots on the surface of accreting neutron stars have been directly observed via pulsations in the lightcurves of X-ray pulsars. They are thought to occur due to magnetic channelling of the accreted fuel to the neutron star magnetic poles. Some X-r
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::989b9568a16bd89ed9a39377cdff9fad
http://arxiv.org/abs/2106.04107
http://arxiv.org/abs/2106.04107
Publikováno v:
Astrophysical Journal, 871(1):61. IOP Publishing Ltd.
Astrophysical Journal 871(2019)1, 61
The Astrophysical Journal
Astrophysical Journal 871(2019)1, 61
The Astrophysical Journal
Accreting neutron stars (NS) can exhibit high-frequency modulations, known as burst oscillations, in their lightcurves during thermonuclear X-ray bursts. Their frequencies can be offset from the spin frequency of the NS (known independently) by sever
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::5db0e1b7164d10f2f6ee7aeb8088a8b6
https://dare.uva.nl/personal/pure/en/publications/burning-in-the-tail(0c9e9189-0d8d-4bb1-a65f-d81103f662ae).html
https://dare.uva.nl/personal/pure/en/publications/burning-in-the-tail(0c9e9189-0d8d-4bb1-a65f-d81103f662ae).html
Publikováno v:
Physical Review Fluids, 4(7):074802. American Physical Society
Physical Review Fluids
UPCommons. Portal del coneixement obert de la UPC
Universitat Politècnica de Catalunya (UPC)
Physical Review Fluids 4(2019), 074802
Physical Review Fluids
UPCommons. Portal del coneixement obert de la UPC
Universitat Politècnica de Catalunya (UPC)
Physical Review Fluids 4(2019), 074802
Convection in rotating spherical geometries is an important physical process in planetary and stellar systems. Using continuation methods at low Prandtl number, we find both strong equatorially asymmetric and symmetric polar nonlinear rotating waves
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::d8d51b6c83ba374461dc2fe39f66bea2
http://arxiv.org/abs/1806.10679
http://arxiv.org/abs/1806.10679
Publikováno v:
Physical Review Fluids. 3
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::392b62869c367019e6ff00207856a79e
https://doi.org/10.1103/physrevfluids.3.059901
https://doi.org/10.1103/physrevfluids.3.059901
Publikováno v:
Physical Review Fluids, 3(2):024801. American Physical Society
Physical Review Fluids
Physical Review Fluids
This study considers the onset of stress-free Boussinesq thermal convection in rotating spherical shells with an aspect ratio η = ri/ro = 0.9 (ri and ro being the inner and outer radius), Prandtl numbers Pr ∈ [10−4,10−1], and Taylor numbers Ta
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::6374421b2903b3e6dfcfc7273e7dc8a9
https://doi.org/10.1103/physrevfluids.3.024801
https://doi.org/10.1103/physrevfluids.3.024801
Publikováno v:
Physical Review Fluids
Physical Review Fluids, 3(12):123501. American Physical Society
Physical Review Fluids, 3(12):123501. American Physical Society
We present an extensive study of Boussinesq thermal convection including a temperature-dependent internal heating source, based on numerical three-dimensional simulations. The temperature dependence mimics triple-$\alpha$ nuclear reactions and the fl
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::cb71a4584a1a6aa136e0c64580a49365
Publikováno v:
Monthly Notices of the Royal Astronomical Society, 477(4), 4391-4402. Oxford University Press
Monthly Notices of the Royal Astronomical Society
Monthly Notices of the Royal Astronomical Society
Accreting neutron stars (NS) can exhibit high frequency modulations in their lightcurves during thermonuclear X-ray bursts, known as burst oscillations. The frequencies can be offset from the spin frequency of the NS by several Hz, and can drift by 1
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::e7c4b8b3ed7a26f494135d970eafa1d5