Zobrazeno 1 - 10
of 261
pro vyhledávání: '"Michael M Woolfson"'
Autor:
Michael M Woolfson
Publikováno v:
Earth, Moon, and Planets. 117:77-91
Estimates of the proportion of Sun-like stars with accompanying planets vary widely; the best present estimate is that it is about 0.34. The capture theory of planet formation involves an interaction between a condensed star and either a diffuse prot
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::7f9c720d2117324ef5af9b726218cde0
https://doi.org/10.1007/s11038-016-9482-5
https://doi.org/10.1007/s11038-016-9482-5
Autor:
Michael M Woolfson
The Capture Theory gives planet production through a tidal interaction between a condensed star and a diffuse protostar within a dense embedded cluster. Initial extensive and highly eccentric planetary orbits round-off and decay in a circumstellar di
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::ae139d6a94764f61cc3bba916ac29250
http://arxiv.org/abs/1709.07294
http://arxiv.org/abs/1709.07294
Autor:
Michael M Woolfson
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 436:1492-1496
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::480c7d1c4c316eff25c1d6d333e3f0d2
https://doi.org/10.1093/mnras/stt1668
https://doi.org/10.1093/mnras/stt1668
Autor:
Michael M Woolfson
Publikováno v:
Earth, Moon, and Planets. 111:1-14
In a scenario produced by the Capture Theory of planetary formation, a collision between erstwhile solar-system giant planets, of masses 798.75 and 598.37 M⊕, is simulated using smoothed-particle hydrodynamics. Due to grain-surface chemistry that t
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::2aead0d5d568a6df417f4e0d138dc510
https://doi.org/10.1007/s11038-013-9420-8
https://doi.org/10.1007/s11038-013-9420-8
Autor:
Michael M Woolfson
Publikováno v:
The Fundamentals of Imaging: From Particles to Galaxies
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::28f2ecf3e7b7fb4e3f7d9c428fe27eaf
https://doi.org/10.1142/9781786340863_0002
https://doi.org/10.1142/9781786340863_0002
Autor:
Michael M Woolfson
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 419:358-365
The collision of uniform gas streams is analysed by the Rankine–Hugoniot equations, which gives a precise description of its behaviour, and also by the computational von Neumann–Richtmeyer (VNR) method. The latter gives large spurious entropy gen
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::083baa769e51447c71a93e7840081538
https://doi.org/10.1111/j.1365-2966.2011.19698.x
https://doi.org/10.1111/j.1365-2966.2011.19698.x
Autor:
Michael M Woolfson
Publikováno v:
Physica Scripta. 93:032501
From its birth in 1912, when only the simplest structures could be solved, x-ray structural crystallography is now able to solve macromolecular structures containing many thousands of independent non-hydrogen atoms. This progress has depended on, and
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::221874dc657528e772691c2698946e62
https://doi.org/10.1088/1402-4896/aa9c30
https://doi.org/10.1088/1402-4896/aa9c30
Autor:
Michael M Woolfson
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 376:1173-1181
Modelling planets is done for two main reasons ‐ the first to further understanding of their internal structure and the second to provide models to explore astrophysical situations in which planets play a role. For the latter reason, the requiremen
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::83856e1e12c54cfcf25be592be8b8d71
https://doi.org/10.1111/j.1365-2966.2007.11498.x
https://doi.org/10.1111/j.1365-2966.2007.11498.x
Autor:
Michael M Woolfson
Publikováno v:
Time and Age: Time Machines, Relativity and Fossils
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::ac2fd0c6684cea6933dd087faaa175e7
https://doi.org/10.1142/9781783265855_0002
https://doi.org/10.1142/9781783265855_0002