2008ApJ...672.1043Y


Query : 2008ApJ...672.1043Y

2008ApJ...672.1043Y - Astrophys. J., 672, 1043-1053 (2008/January-2)

ν-Process nucleosynthesis in population III core-collapse supernovae.

YOSHIDA T., UMEDA H. and NOMOTO K.

Abstract (from CDS):

We investigate the effects of neutrino-nucleus interactions (the ν-process) on the production of iron-peak elements in Population III core-collapse supernovae. The ν-process and the following proton and neutron capture reactions produce odd-Z iron-peak elements in the complete and incomplete Si-burning region. This reaction sequence enhances the abundances of Sc, Mn, and Co in the supernova ejecta. Supernova explosion models of 15 and 25 M☉ stars with the ν-process reproduce well the average Mn/Fe ratio observed in extremely metal-poor halo stars. In order to reproduce the observed Mn/Fe ratio, the total neutrino energy in the supernovae should be 3-9x1053 ergs. Stronger neutrino irradiation and other production sites are necessary to reproduce the observed Sc/Fe and Co/Fe ratios, although these ratios increase by the ν-process.

Abstract Copyright: ∼

Journal keyword(s): Galaxy: Halo - Neutrinos - Nuclear Reactions, Nucleosynthesis, Abundances - Stars: Supernovae: General

Simbad objects: 1

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Number of rows : 1
N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2026
#notes
1 SN 2005bf SN* 10 23 56.99 -03 11 29.3     18.0     SNIb 225 1

Query : 2008ApJ...672.1043Y

Basic data :
SN 2005bf -- SuperNova
Other object types:
otypes_help
SN* (2012A&A,SN)
ICRS coord. (ep=J2000) :
10 23 56.99 -03 11 29.3 [ ] D 2005IAUC.8507....1M
FK4 coord. (ep=B1950 eq=1950) :
10 21 24.72 -02 56 16.1 [ ]
Gal coord. (ep=J2000) :
247.56228 +43.27341 [ ]
Radial velocity / Redshift / cz :
V(km/s) 5613 [~] / z(~) 0.0189 [~] / cz 5666 [~]
   D 2014MNRAS.437.3848L
Spectral type:
SNIb C 2014AJ....147...99M
Fluxes (1) :
V 18.0 [~] D 2008yCat.2283....0B
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SN 2005bf

References (225 between 1850 and 2026) (Total 225)
Simbad bibliographic survey began in 1850 for stars (at least bright stars) and in 1983 for all other objects (outside the solar system).
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