Zobrazeno 1 - 10
of 248
pro vyhledávání: '"A. G. W. Cameron"'
Autor:
D. Ezer, A. G. W. Cameron
Publikováno v:
Solar Neutrinos ISBN: 9780429502811
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::2138bb0a36dbd7e6c9aa4868c63cf9aa
https://doi.org/10.1201/9780429502811-14
https://doi.org/10.1201/9780429502811-14
Autor:
A. G. W. Cameron
Publikováno v:
The Astrophysical Journal. 587:327-340
In a recent work, I have discussed some of the consequences of including rotation and magnetic fields in a model of a core-collapse supernova. Rotation produces equatorial flattening in the resultant neutron star and also produces a surrounding accre
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::e168af627ec7d050ac2c1cd68f324213
https://doi.org/10.1086/368110
https://doi.org/10.1086/368110
Autor:
A. G. W. Cameron
Publikováno v:
The Astrophysical Journal. 562:456-469
In a core-collapse supernova event a rapidly rotating neutron star is formed (in the more massive stars this may subsequently collapse to a black hole). Recent studies have indicated that an intrinsic feature of the subsequent explosion is the flood
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::841c3e5a615a0c8923f6190c68de5fe9
https://doi.org/10.1086/323869
https://doi.org/10.1086/323869
Publikováno v:
Icarus. 150:288-296
We describe a scaling relationship that can be used to characterize the results of numerical smooth particle hydrodynamic (SPH) experiments of potential satellite-forming impacts. The relationship is used to interpret and summarize data from 41 such
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::0e875f435ea529c13168dd70f16a0085
https://doi.org/10.1006/icar.2000.6581
https://doi.org/10.1006/icar.2000.6581
Autor:
A. G. W. Cameron
Publikováno v:
Meteoritics & Planetary Science. 36:9-22
— This paper reports the current status of my smoothed particle hydrodynamic (SPH) simulations of the formation of the Moon. Since the Moon has recently been found to have been formed approximately 50 Ma after the solar nebula itself was formed, I
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::38d3947b5c169d283b8289ec35fc5d89
https://doi.org/10.1111/j.1945-5100.2001.tb01806.x
https://doi.org/10.1111/j.1945-5100.2001.tb01806.x
Autor:
A. G. W. Cameron
Publikováno v:
Annual Review of Astronomy and Astrophysics. 37:1-36
▪ Abstract I was born and educated in Canada, obtaining my PhD in experimental nuclear physics. When I learned that technetium had been found in stellar spectra, I taught myself some astrophysics and began to study stellar nucleosynthesis. This is
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::367c31845acd6b326d61879f76df86a5
https://doi.org/10.1146/annurev.astro.37.1.1
https://doi.org/10.1146/annurev.astro.37.1.1
Autor:
Harri A. T. Vanhala, A. G. W. Cameron
Publikováno v:
The Astrophysical Journal. 508:291-307
Results from numerical simulations of shock waves impacting molecular cloud cores are presented. The three-dimensional smoothed particle hydrodynamics code used in the calculations includes effects from a varying adiabatic exponent, molecular, atomic
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::bfd9b0d6dd95da3e64efc785539a149b
https://doi.org/10.1086/306396
https://doi.org/10.1086/306396
Autor:
A. G. W. Cameron
Publikováno v:
Meteoritics. 30:133-161
— The 26Al/27Al ratio in a large number of calcium-aluminum inclusions (CAIs) is a rather uniform 5 × 10−5, whereas in chondrules the ratio is either undetectable or has a much lower value; the simplest interpretation of this is that there was a
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::72841eb6a9374becbd910bd241fd6d69
https://doi.org/10.1111/j.1945-5100.1995.tb01110.x
https://doi.org/10.1111/j.1945-5100.1995.tb01110.x
Autor:
G W, CAMERON
Publikováno v:
Sewage works journal. 19(4)
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=pmid________::445c33ebaf003370d97ffdd8e78e3107
https://pubmed.ncbi.nlm.nih.gov/20258544
https://pubmed.ncbi.nlm.nih.gov/20258544
Publikováno v:
Icarus. 99:167-174
Simulations of collisions are conducted between a model of the primitive Uranus and 1-3 earth-mass impactors, using smooth-particle hydrodynamics. A series of collisions was simulated for each impactor while varying the total angular momentum of the
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::c220dd0034297c13afb0f5f0cead36e8
https://doi.org/10.1016/0019-1035(92)90180-f
https://doi.org/10.1016/0019-1035(92)90180-f