Zobrazeno 1 - 10
of 41
pro vyhledávání: '"W D Arnett"'
Publikováno v:
Monthly Notices of the Royal Astronomical Society.
Our knowledge of stellar evolution is driven by one-dimensional (1D) simulations. 1D models, however, are severely limited by uncertainties on the exact behaviour of many multi-dimensional phenomena occurring inside stars, affecting their structure a
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::3dd3e5b883d2580b63ee88f3e015a740
https://doi.org/10.1093/mnras/stad1572
https://doi.org/10.1093/mnras/stad1572
Our understanding of stellar structure and evolution coming from one-dimensional (1D) stellar models is limited by uncertainties related to multi-dimensional processes taking place in stellar interiors. 1D models, however, can now be tested and impro
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::8f10f96e20df2c84b03ea3dcf114f4a9
http://arxiv.org/abs/2207.03223
http://arxiv.org/abs/2207.03223
Publikováno v:
AIP Advances, Vol 4, Iss 4, Pp 041010-041010-12 (2014)
Three-dimensional (3D), time dependent numerical simulations of flow of matter in stars, now have sufficient resolution to be fully turbulent. The late stages of the evolution of massive stars, leading up to core collapse to a neutron star (or black
Externí odkaz:
https://doaj.org/article/ce166e3c07974c1ebd7be7aa60a230c7
Autor:
John C. Lattanzio, G. M. De Silva, Simon Campbell, Valentina D'Orazi, Casey Meakin, Dennis Stello, W. D. Arnett, Thomas Constantino, Charles A. Kuehn, B. T. MacLean, Jørgen Christensen-Dalsgaard
Publikováno v:
Astronomische Nachrichten. 337:788-792
Stellar models provide a vital basis for many aspects of astronomy and astro-physics. Recent advances in observational astronomy – through asteroseismology, precision photometry, high-resolution spectroscopy, and large-scale surveys – are placing
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::fcf6ca56cf4ada078551a64f3c85c604
https://doi.org/10.1002/asna.201612373
https://doi.org/10.1002/asna.201612373
Autor:
Sumner Starrfield, Christian Iliadis, Casey Meakin, Warren M. Sparks, W. D. Arnett, Francis Timmes, William Raphael Hix
Publikováno v:
Proceedings of the International Astronomical Union. 7:166-171
We have begun new studies of the evolution of thermonuclear runaways (TNRs) in the accreted envelopes of white dwarfs (WDs). Here we focus on the recent outbursts of RS Oph (2006), U Sco (2010) and T Pyx (2011). U Sco explodes about every 10 years an
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::9e4b67685118467399879fe791520aeb
https://doi.org/10.1017/s1743921312014937
https://doi.org/10.1017/s1743921312014937
Autor:
George A. Kyrala, Tomasz Plewa, H. S. Park, Abbas Nikroo, W. D. Arnett, C.C. Kuranz, D. C. Marion, John Kline, John C Wheeler, B. K. F. Young, R. P. Drake, A. R. Miles, Christine Krauland, Bruce Remington, E. M. Giraldez, F. W. Doss, Harry Robey, J. D. Kilkenny, E. C. Harding, Brian Maddox, E.S. Myra, Christopher J. Keane, Daniel H. Kalantar, Michael Grosskopf, R. J. Wallace, C. M. Huntington
Publikováno v:
Astrophysics and Space Science. 336:207-211
The National Ignition Facility (NIF) is capable of creating new and novel high-energy-density (HED) systems relevant to astrophysics. Specifically, a system could be created that studies the effects of a radiative shock on a hydrodynamically unstable
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::8b6504fa76caa64c936d70b6a6f1ade9
https://doi.org/10.1007/s10509-011-0679-9
https://doi.org/10.1007/s10509-011-0679-9
Autor:
Casey Meakin, Sumner Starrfield, William Raphael Hix, W. D. Arnett, W. M. Sparks, Christian Iliadis, F. X. Timmes
Publikováno v:
Open Astronomy, Vol 21, Iss 1-2, Pp 76-87 (2012)
ResearcherID
NASA Astrophysics Data System
ResearcherID
NASA Astrophysics Data System
Symbiotic binaries are systems containing white dwarfs (WDs) and red giants. Symbiotic novae are those systems in which thermonuclear eruptions occur on the WD components. These are to be distinguished from events driven by accretion disk instabiliti
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::72de8b9db43b010aae694e97001f6778
http://arxiv.org/abs/1211.6145
http://arxiv.org/abs/1211.6145
Publikováno v:
AIP Advances, Vol 4, Iss 4, Pp 041010-041010-12 (2014)
Three-dimensional (3D), time dependent numerical simulations, of flow of matter in stars, now have sufficient resolution to be fully turbulent. The late stages of the evolution of massive stars, leading up to core collapse to a neutron star (or black
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::3e97b623795c0fa8e104b5a63ca5bc14
https://doaj.org/article/ce166e3c07974c1ebd7be7aa60a230c7
https://doaj.org/article/ce166e3c07974c1ebd7be7aa60a230c7
Autor:
W. D. Arnett
Publikováno v:
Communications of the ACM. 28:354-357
As computers become more powerful and sophisticated, computational astrophysicists will be able to find out more about stellar evolution and other astronomical phenomena.
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::b2252756223e8a857925f74885b2192d
https://doi.org/10.1145/3341.3342
https://doi.org/10.1145/3341.3342
Publikováno v:
Canadian Journal of Physics. 45:2315-2332
It is generally assumed that element synthesis will take place readily under the extreme conditions believed to exist in supernova explosions. We have examined the types of thermonuclear reactions that can occur in a supernova shock wave which propag
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::59fd8f8055818a55e3cec27b10457ba4
https://doi.org/10.1139/p67-184
https://doi.org/10.1139/p67-184