Zobrazeno 1 - 6
of 6
pro vyhledávání: '"Friedrich-K. Thielemann"'
Various nucleosynthesis studies have pointed out that the rapid neutron capture r-process elements in very metal-poor (VMP) halo stars might have different origins. It has been known that an r-process can either be obtained in neutron-rich low Ye con
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::c347d569c5a0d900edad2d162f8aa921
https://edoc.unibas.ch/92930/
https://edoc.unibas.ch/92930/
Autor:
A. Hujeirat, Friedrich-K. Thielemann
Publikováno v:
NASA Astrophysics Data System
Einleitung Kurz nach dem zweiten Weltkrieg waren Rudolf Kippenhahn, damals in Erlangen/Bamberg und spater Professor in Gottingen bzw. Direktor des Max-Planck-Instituts fur Astrophysik, sowie Martin Schwarzschild, der in Gottingen promoviert hatte und
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::6c4a339260174b811611bf0f0ef69be2
https://doi.org/10.1007/s00287-009-0391-0
https://doi.org/10.1007/s00287-009-0391-0
Autor:
Friedrich-K. Thielemann
Publikováno v:
Hadrons, Nuclei and Applications.
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::72596e5a193e275d24f67c6d2a5b9264
https://doi.org/10.1142/9789812810922_0046
https://doi.org/10.1142/9789812810922_0046
Autor:
Koichi Iwamoto, Hideyuki Umeda, M. R. Strayer, D. J. Dean, K. Langanke, Gabriel Martínez-Pinedo, W. Raphael Hix, Ken'ichi Nomoto, F. Brachwitz, Friedrich-K. Thielemann
Publikováno v:
Brachwitz, F, Dean, D J, Hix, W R, Iwamoto, K, Langanke, K, Martinez-Pinedo, G, Nomoto, K, Strayer, M R, Thielemann, F-K & Umeda, H 2000, ' The role of electron captures in Chandrasekhar mass models for type Ia supernovae ', Astr. Journal, vol. 536, pp. 934 .
The Chandrasekhar mass model for Type Ia Supernovae (SNe Ia) has received increasing support from recent comparisons of observations with light curve predictions and modeling of synthetic spectra. It explains SN Ia events via thermonuclear explosions
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::a464a19f5681424c4dcc6d2e59b8bbfe
Publikováno v:
Astrophysics and Space Science. 118:305-309
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::f44a1c6f6b5bfdb487987f08a3624e26
https://doi.org/10.1007/bf00651141
https://doi.org/10.1007/bf00651141
Publikováno v:
Third Asian-Pacific Regional Meeting of the International Astronomical Union ISBN: 9789401085038
A carbon deflagration model in the accreting C + O white dwarf is presented as a plausible model for type-I supernovae (SN I). The evolution of the white dwarf is calculated from the beginning of accretion through complete disruption. The propagation
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::acbcc49a59210a8233e73aae6790d34a
https://doi.org/10.1007/978-94-009-4496-1_46
https://doi.org/10.1007/978-94-009-4496-1_46