S-process nucleosynthesis in AGB stars with the full spectrum of turbulence scheme for convection.

被引：1

作者：

Yague, A. ^{[1
,2
,3
]}

Garcia-Hernandez, D. A. ^{[2
,3
]}

Ventura, P. ^{[1
]}

Lugaro, M. ^{[4
,5
]}

机构：

[1] Ist Nazl Astrofis OAR, Monte Porzio Catone, Italy

[2] Inst Astrofis Canarias, Tenerife, Spain

[3] Univ La Laguna, Dept Astrofis, Tenerife, Spain

[4] Hungarian Acad Sci, Konkoly Observ, Budapest, Hungary

[5] Monash Univ, Monash Ctr Astrophys, Clayton, Vic, Australia

来源：

11TH PACIFIC RIM CONFERENCE ON STELLAR ASTROPHYSICS: PHYSICS AND CHEMISTRY OF THE LATE STAGES OF STELLAR EVOLUTION, PTS 1-6 | 2016年 / 728卷

关键词：

LITHIUM PRODUCTION; RUBIDIUM;

D O I：

10.1088/1742-6596/728/7/072004

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

The chemical evolution of asymptotic giant branch (AGB) stars models depends greatly on the input physics (e.g. convective model, mass loss recipe). Variations of hot bottom burning (HBB) strength, or third dredge-up (TDU) efficiency are among the main consequences of adopting different input physics in the AGB models. The ATON evolutionary code stands apart from others in that it uses the Full Spectrum of Turbulence convective model. Here we present the first results of a newly developed s-process nucleosynthesis module for ATON AGB models. Our results are compared also with observations and theoretical predictions of present AGB nucleosynthesis models using different input physics.

引用

页数：2

共 50 条

[1] S-process nucleosynthesis in primordial AGB stars
Siess, L
Goriely, S
NUCLEAR PHYSICS A, 2003, 718 : 524C - 526C
[2] Evolution of rotating AGB stars and the s-process nucleosynthesis
Siess, L
Goriely, S
Langer, N
PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF AUSTRALIA, 2003, 20 (04): : 371 - 377
[3] MONTAGE: AGB Nucleosynthesis with Full s-Process Calculations
Church, R. P.
Cristallo, S.
Lattanzio, J. C.
Stancliffe, R. J.
Straniero, O.
Cannon, R. C.
PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF AUSTRALIA, 2009, 26 (03): : 217 - 224
[4] Sensitivity of the s-process nucleosynthesis in AGB stars to the overshoot model
Goriely, S.
Siess, L.
ASTRONOMY & ASTROPHYSICS, 2018, 609
[5] Post-AGB Stars in the Magellanic Clouds as Tracers of the s-Process Nucleosynthesis
De Smedt, K.
Van Winckel, H.
Kamath, D.
Karakas, A. I.
Siess, L.
Goriely, S.
Wood, P. R.
WHY GALAXIES CARE ABOUT AGB STARS III: A CLOSER LOOK IN SPACE AND TIME, 2015, 497 : 241 - 246
[6] Barium stars as tracers of s-process nucleosynthesis in AGB stars I. 28 stars with independently derived AGB mass
Cseh, B.
Vilagos, B.
Roriz, M. P.
Pereira, C. B.
D'Orazi, V
Karakas, A., I
Soos, B.
Drake, N. A.
Junqueira, S.
Lugaro, M.
ASTRONOMY & ASTROPHYSICS, 2022, 660
[7] Barium stars as tracers of s-process nucleosynthesis in AGB stars III. Systematic deviations from the AGB models
Vilagos, B.
Cseh, B.
Lopez, A. Yague
Joyce, M.
Karakas, A.
Tagliente, G.
Lugaro, M.
ASTRONOMY & ASTROPHYSICS, 2024, 688
[8] S-process Nucleosynthesis in SAGB Stars
Lau, H. H. B.
Doherty, C. L.
Gil-Pons, P.
Lattanzio, J. C.
WHY GALAXIES CARE ABOUT AGB STARS II: SHINING EXAMPLES AND COMMON INHABITANTS, 2011, 445 : 45 - +
[9] The s-process in rotating AGB stars
Herwig, F
Langer, N
Lugaro, M
PLANETARY NEBULAE: THEIR EVOLUTION AND ROLE IN THE UNIVERSE, 2003, (209): : 99 - 100
[10] s-process nucleosynthesis in carbon stars
Abia, C
Domínguez, I
Gallino, R
Busso, M
Masera, S
Straniero, O
de Laverny, P
Plez, B
Isern, J
ASTROPHYSICAL JOURNAL, 2002, 579 (02): : 817 - 831

← 1 2 3 4 5 →