1999ApJ...511L..33I


Query : 1999ApJ...511L..33I

1999ApJ...511L..33I - Astrophys. J., 511, L33-L36 (1999/January-3)

Enrichment of the r-process element europium in the galactic halo.

ISHIMARU Y. and WANAJO S.

Abstract (from CDS):

We investigate the enrichment of europium, as a representative of r-process elements, in the Galactic halo. In present chemical evolution models, stars are assumed to be formed through shock processes by supernovae (SNe). The enrichment of the interstellar medium is calculated by a one-zone approach. The observed large dispersions in [Eu/Fe] for halo stars, converging with increasing metallicity, can be explained with our models. In addition, the mass range of SNe for the r-process site is constrained to be either stars of 8-10 or ≳30 M☉.

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

Simbad objects: 6

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Number of rows : 6
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 1997D SN* 04 11 01.00 -56 29 56.0       16.3   SNIIpec 184 1
2 SN 1994W SN* 12 02 10.92 +62 08 32.7     13.3     SNIInP 194 1
3 HD 115444 Pe* 13 16 42.4590842616 +36 22 52.692135420   9.77 8.97 8.3 7.88 G9V 252 0
4 HD 122563 Pe* 14 02 31.8455084952 +09 41 09.944391876 7.47 7.10 6.19 5.37 4.79 G8:III:Fe-5 920 0
5 HD 126238 Pe* 14 25 29.9571431040 -43 38 36.948515460   8.44 7.7 7.44   G3/8wF0/2 119 0
6 BPS CS 22892-0052 Pe* 22 17 01.6558764360 -16 39 27.051026544   14.03 13.20 13.06 12.19 KIIvw 472 0

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