Zobrazeno 1 - 10
of 34
pro vyhledávání: '"Otsuki, Kaori"'
Publikováno v:
Astron.Astrophys.471:227-236,2007
We explore heavy-element nucleosynthesis by rapid neutron capture (r-process) in the decompressing ejecta from the surface of a neutron star. The decompression is triggered by a violent phase transition to strange quark matter (quark-nova scenario).
Externí odkaz:
http://arxiv.org/abs/nucl-th/0610013
Publikováno v:
Astrophys.J. 641 (2006) L117-L120
We report on observations of six giants in the globular cluster M15 (NGC 7078) using the Subaru Telescope to measure neutron-capture elemental abundances. Our abundance analyses based on high-quality blue spectra confirm the star-to-star scatter in t
Externí odkaz:
http://arxiv.org/abs/astro-ph/0603328
We review recent observational and theoretical results concerning the presence of actinide nuclei on the surfaces of old halo stars and their use as an age determinant. We present model calculations which show that the observed universality of abunda
Externí odkaz:
http://arxiv.org/abs/astro-ph/0207596
We present calculations of r-process nucleosynthesis in neutrino-driven winds from the nascent neutron stars of core-collapse supernovae. A full dynamical reaction network for both the alpha-rich freezeout and the subsequent r-process is employed. Th
Externí odkaz:
http://arxiv.org/abs/astro-ph/0102261
We study the few body reactions in explosive nucleosynthesis of light-to-heavy mass elements in various astrophysical conditions. In neutrino-driven winds of gravitational core collapse of SNeII, several light nuclei as well as heavy unstable nuclei
Externí odkaz:
http://arxiv.org/abs/astro-ph/0006079
Neutrino-driven wind from young hot neutron star, which is formed by supernova explosion, is the most promising candidate site for r-process nucleosynthesis. We study general relativistic effects on this wind in Schwarzschild geometry in order to loo
Externí odkaz:
http://arxiv.org/abs/astro-ph/9911164
The gravitaional force produced by a point particle, like the sun, in the background of the static Einstein universe is studied. Both the approximate solution in the weak field limit and exact solution are obtained. The main properties of the solutio
Externí odkaz:
http://arxiv.org/abs/gr-qc/9405017
Publikováno v:
In New Astronomy 2003 8(8):767-776
Publikováno v:
福岡大学理学集報 = Fukuoka University Science Reports. 45(1):9-13
Autor:
Truran, James W., Otsuki, Kaori
Publikováno v:
Proceedings of the International Astronomical Union. 05/03/2005, Vol. 1 Issue S228, p421-428. 8p.