scholarly journals Neutron Capture in Low‐Mass Asymptotic Giant Branch Stars: Cross Sections and Abundance Signatures

1999 ◽  
Vol 525 (2) ◽  
pp. 886-900 ◽  
Author(s):  
Claudio Arlandini ◽  
Franz Kappeler ◽  
Klaus Wisshak ◽  
Roberto Gallino ◽  
Maria Lugaro ◽  
...  

1998 ◽  
Vol 497 (1) ◽  
pp. 388-403 ◽  
Author(s):  
Roberto Gallino ◽  
Claudio Arlandini ◽  
Maurizio Busso ◽  
Maria Lugaro ◽  
Claudia Travaglio ◽  
...  


1997 ◽  
Vol 478 (1) ◽  
pp. 332-339 ◽  
Author(s):  
Oscar Straniero ◽  
Alessandro Chieffi ◽  
Marco Limongi ◽  
Maurizio Busso ◽  
Roberto Gallino ◽  
...  


2014 ◽  
Vol 790 (1) ◽  
pp. 22 ◽  
Author(s):  
Philip Rosenfield ◽  
Paola Marigo ◽  
Léo Girardi ◽  
Julianne J. Dalcanton ◽  
Alessandro Bressan ◽  
...  


Science ◽  
2014 ◽  
Vol 345 (6197) ◽  
pp. 650-653 ◽  
Author(s):  
Maria Lugaro ◽  
Alexander Heger ◽  
Dean Osrin ◽  
Stephane Goriely ◽  
Kai Zuber ◽  
...  

Among the short-lived radioactive nuclei inferred to be present in the early solar system via meteoritic analyses, there are several heavier than iron whose stellar origin has been poorly understood. In particular, the abundances inferred for 182Hf (half-life = 8.9 million years) and 129I (half-life = 15.7 million years) are in disagreement with each other if both nuclei are produced by the rapid neutron-capture process. Here, we demonstrate that contrary to previous assumption, the slow neutron-capture process in asymptotic giant branch stars produces 182Hf. This has allowed us to date the last rapid and slow neutron-capture events that contaminated the solar system material at ∼100 million years and ∼30 million years, respectively, before the formation of the Sun.



2004 ◽  
Vol 602 (1) ◽  
pp. 377-387 ◽  
Author(s):  
Nobuyuki Iwamoto ◽  
Toshitaka Kajino ◽  
Grant J. Mathews ◽  
Masayuki Y. Fujimoto ◽  
Wako Aoki


2009 ◽  
Vol 696 (1) ◽  
pp. 797-820 ◽  
Author(s):  
S. Cristallo ◽  
O. Straniero ◽  
R. Gallino ◽  
L. Piersanti ◽  
I. Domínguez ◽  
...  


1988 ◽  
Vol 334 ◽  
pp. L45 ◽  
Author(s):  
R. Gallino ◽  
M. Busso ◽  
G. Picchio ◽  
C. M. Raiteri ◽  
A. Renzini




2018 ◽  
Vol 14 (S343) ◽  
pp. 510-511
Author(s):  
G. Tautvaišienė ◽  
C. Viscasillas Vázquez ◽  
V. Bagdonas ◽  
R. Smiljanic ◽  
A. Drazdauskas ◽  
...  

AbstractAsymptotic giant branch stars play an important role in enriching galaxies by s-process elements. Recent studies have shown that their role in producing s-process elements in the Galactic disc was underestimated and should be reconsidered. Based on high-resolution spectra we have determined abundances of neutron-capture elements in a sample of 310 stars located in the field and open clusters and investigated elemental enrichment patterns according to their age and mean galactocentric distances.



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