Roberto Gallino
Roberto Gallino
Professor of Physics, University of Turin, Italy
Bestätigte E-Mail-Adresse bei
Zitiert von
Zitiert von
Nucleosynthesis in asymptotic giant branch stars: Relevance for galactic enrichment and solar system formation
M Busso, R Gallino, GJ Wasserburg
Annual Review of Astronomy and Astrophysics 37 (1), 239-309, 1999
Evolution and nucleosynthesis in low-mass asymptotic giant branch stars. II. Neutron capture and the s-process
R Gallino, C Arlandini, M Busso, M Lugaro, C Travaglio, O Straniero, ...
The astrophysical journal 497 (1), 388, 1998
Neutron capture in low-mass asymptotic giant branch stars: cross sections and abundance signatures
C Arlandini, F Käppeler, K Wisshak, R Gallino, M Lugaro, M Busso, ...
The Astrophysical Journal 525 (2), 886, 1999
Neutron-capture elements in the early galaxy
C Sneden, JJ Cowan, R Gallino
Annu. Rev. Astron. Astrophys. 46, 241-288, 2008
The process: Nuclear physics, stellar models, and observations
F Käppeler, R Gallino, S Bisterzo, W Aoki
Reviews of Modern Physics 83 (1), 157, 2011
Galactic evolution of Sr, Y, and Zr: a multiplicity of nucleosynthetic processes
C Travaglio, R Gallino, E Arnone, J Cowan, F Jordan, C Sneden
The Astrophysical Journal 601 (2), 864, 2004
Evolution, nucleosynthesis, and yields of low-mass asymptotic giant branch stars at different metallicities. II. The FRUITY database
S Cristallo, L Piersanti, O Straniero, R Gallino, I Domínguez, C Abia, ...
The Astrophysical Journal Supplement Series 197 (2), 17, 2011
Nucleosynthesis and mixing on the asymptotic giant branch. III. Predicted and observed s-process abundances
M Busso, R Gallino, DL Lambert, C Travaglio, VV Smith
The Astrophysical Journal 557 (2), 802, 2001
Radiative C-13 burning in asymptotic giant branch stars and s-processing
O Straniero, R Gallino, M Busso, A Chiefei, CM Raiteri, M Limongi, ...
Astrophysical Journal, Part 2-Letters (ISSN 0004-637X), vol. 440, no. 2, p …, 1995
The weak s-process in massive stars and its dependence on the neutron capture cross sections
M Pignatari, R Gallino, M Heil, M Wiescher, F Käppeler, F Herwig, ...
The Astrophysical Journal 710 (2), 1557, 2010
Abundances of actinides and short-lived nonactinides in the interstellar medium: diverse supernova sources for the r-processes
GJ Wasserburg, M Busso, R Gallino
The Astrophysical Journal 466 (2), L109, 1996
Evolution and nucleosynthesis in low-mass asymptotic giant branch stars. I. Formation of population I carbon stars
O Straniero, A Chieffi, M Limongi, M Busso, R Gallino, C Arlandini
The Astrophysical Journal 478 (1), 332, 1997
Galactic chemical evolution of heavy elements: from barium to europium
C Travaglio, D Galli, R Gallino, M Busso, F Ferrini, O Straniero
The Astrophysical Journal 521 (2), 691, 1999
s process in low-mass asymptotic giant branch stars
O Straniero, R Gallino, S Cristallo
Nuclear Physics A 777, 311-339, 2006
Short-lived nuclei in the early Solar System: Possible AGB sources
GJ Wasserburg, M Busso, R Gallino, KM Nollett
Nuclear Physics A 777, 5-69, 2006
The chemical evolution of the globular cluster ω Centauri (NGC 5139)
VV Smith, NB Suntzeff, K Cunha, R Gallino, M Busso, DL Lambert, ...
The Astronomical Journal 119 (3), 1239, 2000
s-process nucleosynthesis in asymptotic giant branch stars: A test for stellar evolution
M Lugaro, F Herwig, JC Lattanzio, R Gallino, O Straniero
The astrophysical journal 586 (2), 1305, 2003
Galactic chemical evolution and solar s-process abundances: Dependence on the 13C-pocket structure
S Bisterzo, C Travaglio, R Gallino, M Wiescher, F Käppeler
The Astrophysical Journal 787 (1), 10, 2014
The weak s-component and nucleosynthesis in massive stars
CM Raiteri, R Gallino, M Busso, D Neuberger, F Käppeler
Astrophysical Journal v. 419, p. 207 419, 207, 1993
Isotopic compositions of strontium, zirconium, molybdenum, and barium in single presolar SiC grains and asymptotic giant branch stars
M Lugaro, AM Davis, R Gallino, MJ Pellin, O Straniero, F Käppeler
The Astrophysical Journal 593 (1), 486, 2003
Das System kann den Vorgang jetzt nicht ausführen. Versuchen Sie es später erneut.
Artikel 1–20