Zobrazeno 1 - 10
of 38
pro vyhledávání: '"Brachwitz, F."'
Autor:
Thielemann, F. -K., Argast, D., Brachwitz, F., Martinez-Pinedo, G., Oechslin, R., Rauscher, T., Hix, W. R., Liebendoerfer, M., Mezzacappa, A., Hoeflich, P., Iwamoto, K., Nomoto, K., Schatz, H., Wiescher, M. C., Kratz, K. -L., Pfeiffer, B., Rosswog, S.
With the exception of the Big Bang, responsible for 1,2H, 3,4He, and 7Li, stars act as sources for the composition of the interstellar medium. Cosmic rays are related to the latter and very probably due to acceleration of the mixed interstellar mediu
Externí odkaz:
http://arxiv.org/abs/astro-ph/0202453
Autor:
Thielemann, F. -K., Brachwitz, F., Freiburghaus, C., Kolbe, E., Martinez-Pinedo, G., Rauscher, T., Rembges, F., Hix, W. R., Liebendoerfer, M., Mezzacappa, A., Kratz, K. -L., Pfeiffer, B., Langanke, K., Nomoto, K., Rosswog, S., Schatz, H., Wiescher, M.
Publikováno v:
Prog.Part.Nucl.Phys.46:5-22,2001
Except for 1H, 2H, 3He, 4He, and 7Li, originating from the Big Bang, all heavier elements are made in stellar evolution and stellar explosions. Nuclear physics, and in many cases nuclear structure far from stability, enters in a crucial way. Therefor
Externí odkaz:
http://arxiv.org/abs/astro-ph/0101476
Autor:
Iwamoto, K., Brachwitz, F., Nomoto, K., Kishimoto, N., Umeda, H., Hix, W. R., Thielemann, F. -K.
Publikováno v:
Astrophys.J.Suppl. 125 (2000) 439-462
We calculate explosive nucleosynthesis in Chandrasekhar mass models for Type Ia Supernovae(SNe Ia) to obtain new constraints on the rate of matter accretion onto the progenitor white dwarf and on the ignition density of central carbon deflagration. T
Externí odkaz:
http://arxiv.org/abs/astro-ph/0002337
Autor:
Nomoto, K., Iwamoto, K., Nakasato, N., Thielemann, F. -K., Brachwitz, F., Tsujimoto, T., Kubo, Y., Kishimoto, N.
Among the major uncertainties involved in the Chandrasekhar mass models for Type Ia supernovae are the companion star of the accreting white dwarf (or the accretion rate that determines the carbon ignition density) and the flame speed after ignition.
Externí odkaz:
http://arxiv.org/abs/astro-ph/9706025
Publikováno v:
In New Astronomy Reviews 2004 48(7):605-610
Autor:
Friedrich-Karl Thielemann, Argast, D., Brachwitz, F., Martinez-Pinedo, G., Oechslin, R., Rauscher, T., Hix, W. R., Liebendörfer, M., Mezzacappa, A., Höflich, P., Iwamoto, K., Nomoto, K., Schatz, H., Wiescher, M. C., Kratz, K. -L, Pfeiffer, B., Rosswog, S.
Publikováno v:
NASA Astrophysics Data System
With the exception of the Big Bang, responsible for 1,2H, 3,4He, and 7Li, stars act as sources for the composition of the interstellar medium. Cosmic rays are related to the latter and very probably due to acceleration of the mixed interstellar mediu
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::74a1c547e1ebaae5e829dbadbf353269
http://arxiv.org/abs/astro-ph/0202453
http://arxiv.org/abs/astro-ph/0202453
Autor:
Thielemann, F.K., Brachwitz, F., Freiburghaus, C., Rosswog, S., Iwamoto, K., Nakamura, T., Nomoto, K., Umeda, H., Langanke, Karlheinz, Martinez-Pinedo, G., Dean, D.J., Hix, W.R., Strayer, M.R.
Publikováno v:
Thielemann, F K, Brachwitz, F, Freiburghaus, C, Rosswog, S, Iwamoto, K, Nakamura, T, Nomoto, K, Umeda, H, Langanke, K, Martinez-Pinedo, G, Dean, D J, Hix, W R & Strayer, M R 2001, Abundances in Supernovae . in M Livio (ed.), Proceedings of the international conference on The biggest Explosions in the Universe, Gamma-Ray Bursts and Supernovae . Cambridge University Press, pp. 012703-1-11, 17/12/2010 .
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=pure_au_____::665575598d5b6acc221a9dfb41eb212e
https://pure.au.dk/portal/da/publications/abundances-in-supernovae(017247e0-7ec7-11db-bee9-02004c4f4f50).html
https://pure.au.dk/portal/da/publications/abundances-in-supernovae(017247e0-7ec7-11db-bee9-02004c4f4f50).html
Autor:
Hillebrandt, Wolfgang, Leibundgut, Bruno, Thielemann, F.-K., Argast, D., Brachwitz, F., Hix, W. R., Höflich, P., Liebendörfer, M., Martinez-Pinedo, G., Mezzacappa, A., Nomoto, K., Panov, I.
Publikováno v:
From Twilight to Highlight: The Physics of Supernovae; 2003, p331-343, 13p
Publikováno v:
AIP Conference Proceedings; 2001, Vol. 598 Issue 1, p239, 6p
Autor:
THIELEMANN, F.-K., ARGAST, D., BRACHWITZ, F., GERHARD, O. E., MARTINEZ-PINEDO, G., SAMLAND, M., HIX, W. R., LIEBENDÖRFER, M., MEZZACAPPA, A., NOMOTO, K., NAKAMURA, T., UMEDA, H., IWAMOTO, K.
Publikováno v:
Cosmic Evolution; 2001, p161-169, 9p