22Ne and 23Na ejecta from intermediate-mass stars: the impact of the new LUNA rate for 22Ne(p,γ)23Na
暂无分享,去创建一个
H Germany | -INAF | Italy. | Hungary. | A. Bressan | Infn | Helmholtz-Zentrum Dresden-Rossendorf | United Kingdom. | Trieste | F. Pantaleo | Inst. for Nucl. Research | Supa | U. Milano | M. Junker | C. Gustavino | U. Edinburgh | P. Marigo | D. Bemmerer | Sissa | F. Ferraro | O. Straniero | T. Davinson | G. F. Ciani | L’Aquila | A. Slemer | P. Prati | U. Genova | R. Menegazzo | D. Padova | A. Caciolli | G. Gervino | M. Aliotta | A. Boeltzig | A. Best | C. Broggini | P. Corvisiero | R. Depalo | Z. Elekes | A. Formicola | A. Guglielmetti | G. Imbriani | F. Cavanna | A. Leva | V. Mossa | D. Piatti | C.G.Bruno | Z. p | G. G. rky | T. S. cs | M. Cs | I. Padova | University of Florence ans Infn | Gran Sasso Science Institute | Lngs | University ofTorino | S. Sapienza | U. Bari | O. D. Teramo | T. Cs | F. Pantaleo | Z. P. | G. Ciani | Zs. F l p | T. cs | University of Padua Infn
[1] G. Meynet,et al. Evolution of long-lived globular cluster stars III. Effect of the initial helium spread on the position of stars in a synthetic Hertzsprung-Russell diagram , 2016, 1606.01899.
[2] Alessandro Bressan,et al. EVOLUTION OF THERMALLY PULSING ASYMPTOTIC GIANT BRANCH STARS. V. CONSTRAINING THE MASS LOSS AND LIFETIMES OF INTERMEDIATE-MASS, LOW-METALLICITY AGB STARS , 2016, 1603.05283.
[3] A. Milone,et al. A single model for the variety of multiple-population formation(s) in globular clusters: a temporal sequence , 2016, 1602.05412.
[4] F. Pantaleo,et al. Three New Low-Energy Resonances in the ^{22}Ne(p,γ)^{23}Na Reaction. , 2015, Physical review letters.
[5] J. Anderson,et al. The Hubble Space TelescopeUV Legacy Survey of Galactic Globular Clusters – V. Constraints on formation scenarios , 2015, 1510.01468.
[6] J. Hron,et al. Why galaxies care about AGB stars III : a closer look in space and time : proceedings of a conference held at University campus, Vienna, Austria, 28 July-1 August 2014 , 2015 .
[7] R. Peletier,et al. Why Galaxies Care about AGB Stars III: A Closer Look in Space and Time , 2015 .
[8] E. Carretta,et al. FIVE GROUPS OF RED GIANTS WITH DISTINCT CHEMICAL COMPOSITION IN THE GLOBULAR CLUSTER NGC 2808 , 2015, 1507.07553.
[9] S. Cristallo,et al. EVOLUTION, NUCLEOSYNTHESIS, AND YIELDS OF AGB STARS AT DIFFERENT METALLICITIES. III. INTERMEDIATE-MASS MODELS, REVISED LOW-MASS MODELS, AND THE pH-FRUITY INTERFACE , 2015, 1507.07338.
[10] G. Mattei,et al. Strengths of the resonances at 436, 479, 639, 661, and 1279 keV in the Ne 22 ( p , γ ) Na 23 reaction , 2015, 1507.03893.
[11] N. Bastian,et al. A general abundance problem for all self-enrichment scenarios for the origin of multiple populations in globular clusters , 2015, 1503.03071.
[12] F. Grundahl,et al. CNO abundances in the globular clusters NGC 1851 and NGC 6752 , 2014, 1411.1474.
[13] P. Marigo. Calibrating the role of TP-AGB stars in the cosmic matter cycle , 2014, 1411.3126.
[14] M. Menzel,et al. A new study of the 22Ne(p, γ)23Na reaction deep underground: Feasibility, setup and first observation of the 186 keV resonance , 2014, 1411.2888.
[15] L. Girardi,et al. EVOLUTION OF THERMALLY PULSING ASYMPTOTIC GIANT BRANCH STARS. IV. CONSTRAINING MASS LOSS AND LIFETIMES OF LOW MASS, LOW METALLICITY AGB STARS , 2014, 1406.0676.
[16] J. Lattanzio,et al. The Dawes Review 2: Nucleosynthesis and Stellar Yields of Low- and Intermediate-Mass Single Stars , 2014, Publications of the Astronomical Society of Australia.
[17] J. Lattanzio,et al. Super and massive AGB stars – III. Nucleosynthesis in metal-poor and very metal-poor stars – Z = 0.001 and 0.0001 , 2014, 1403.5054.
[18] D. A. García-Hernández,et al. Circumstellar effects on the Rb abundances in O-rich AGB stars , 2014, 1403.2075.
[19] S. Cristallo,et al. HEAVY ELEMENTS IN GLOBULAR CLUSTERS: THE ROLE OF ASYMPTOTIC GIANT BRANCH STARS , 2014, 1403.0819.
[20] Jason S. Kalirai,et al. THE CORE MASS GROWTH AND STELLAR LIFETIME OF THERMALLY PULSING ASYMPTOTIC GIANT BRANCH STARS , 2013, 1312.4544.
[21] A. Dotter,et al. GLOBAL AND NONGLOBAL PARAMETERS OF HORIZONTAL-BRANCH MORPHOLOGY OF GLOBULAR CLUSTERS , 2013, 1312.4169.
[22] F. Hartwick,et al. Supermassive stars as a source of abundance anomalies of proton-capture elements in globular clusters , 2013, 1305.5975.
[23] R. Longland,et al. Measurement of the e r c.m. = 138 keV resonance in the 23 Na(p, γ) 24 Mg reaction and the abundance of sodium in AGB stars , 2013 .
[24] J. Lattanzio,et al. Super and massive AGB stars - II. Nucleosynthesis and yields - Z = 0.02, 0.008 and 0.004 , 2013, 1310.2614.
[25] M. L. Pumo,et al. Evolution of thermally pulsing asymptotic giant branch stars - I. The COLIBRI code , 2013, 1305.4485.
[26] J. Lattanzio,et al. On the internal pollution mechanisms in the globular cluster NGC 6121 (M4): heavy-element abundances and AGB models ⋆ , 2013, 1304.7009.
[27] M. Criscienzo,et al. Yields of AGB and SAGB models with chemistry of low- and high-metallicity globular clusters , 2013, 1303.3912.
[28] G. Meynet,et al. Superbubble dynamics in globular cluster infancy II. Consequences for secondary star formation in the context of self-enrichment via fast rotating massive stars , 2013, 1302.2494.
[29] P. Bogdanovich,et al. Atomic Data and Nuclear Data Tables , 2013 .
[30] R. Menegazzo,et al. IMPACT OF A REVISED 25Mg(p, γ)26Al REACTION RATE ON THE OPERATION OF THE Mg–Al CYCLE , 2012, 1211.6661.
[31] L. Girardi,et al. parsec: stellar tracks and isochrones with the PAdova and TRieste Stellar Evolution Code , 2012, 1208.4498.
[32] P. Ventura,et al. The role of super-asymptotic giant branch ejecta in the abundance patterns of multiple populations in globular clusters , 2012, 1203.4992.
[33] J. Anderson,et al. Luminosity and mass functions of the three main sequences of the globular cluster NGC 2808 , 2011, 1108.2391.
[34] F. Timmes,et al. STARLIB: A NEXT-GENERATION REACTION-RATE LIBRARY FOR NUCLEAR ASTROPHYSICS , 2011, 1304.7811.
[35] C. Conroy. ON THE BIRTH MASSES OF THE ANCIENT GLOBULAR CLUSTERS , 2011, 1101.2208.
[36] Alessandra Guglielmetti,et al. LUNA: Nuclear Astrophysics Deep Underground , 2010, 1010.4165.
[37] Benjamin F. Williams,et al. THE ACS NEARBY GALAXY SURVEY TREASURY. IX. CONSTRAINING ASYMPTOTIC GIANT BRANCH EVOLUTION WITH OLD METAL-POOR GALAXIES , 2010, 1009.4618.
[38] P. Ventura,et al. Asymptotic giant branch stars at low metallicity: the challenging interplay between the mass-loss and molecular opacities , 2010, 1007.2533.
[39] Ryan M. Ferguson,et al. THE JINA REACLIB DATABASE: ITS RECENT UPDATES AND IMPACT ON TYPE-I X-RAY BURSTS , 2010, The Astrophysical Journal Supplement Series.
[40] S. McMillan,et al. Abundance patterns of multiple populations in globular clusters: a chemical evolution model based on yields from AGB ejecta , 2010, 1005.1892.
[41] Richard Longland,et al. Charged-particle thermonuclear reaction rates: III. Nuclear physics input , 2010, 1004.4149.
[42] R. Longland,et al. Charged-particle thermonuclear reaction rates: II. Tables and graphs of reaction rates and probability density functions , 2010, 1004.4517.
[43] Bernd Freytag,et al. Solar Chemical Abundances Determined with a CO5BOLD 3D Model Atmosphere , 2010, 1003.1190.
[44] Lionel Siess,et al. Evolution of massive AGB stars - III. the thermally pulsing super-AGB phase , 2010 .
[45] A. Karakas. Updated stellar yields from asymptotic giant branch models , 2009, 0912.2142.
[46] S. D. Mink,et al. Massive binaries as the source of abundance anomalies in globular clusters , 2009, 0910.1086.
[47] D. A. García-Hernández,et al. Rb-RICH ASYMPTOTIC GIANT BRANCH STARS IN THE MAGELLANIC CLOUDS , 2009, 0909.4391.
[48] Garching,et al. Na-O anticorrelation and HB - VIII. Proton-capture elements and metallicities in 17 globular clusters from UVES spectra , 2009, 0909.2941.
[49] Austria,et al. Low-temperature gas opacity. ÆSOPUS: a versatile and quick computational tool , 2009, 0907.3248.
[50] H. Costantini,et al. LUNA: a laboratory for underground nuclear astrophysics , 2009, 0906.1097.
[51] S. Cristallo,et al. EVOLUTION, NUCLEOSYNTHESIS, AND YIELDS OF LOW-MASS ASYMPTOTIC GIANT BRANCH STARS AT DIFFERENT METALLICITIES , 2009, 1109.1176.
[52] P. Ventura,et al. Massive AGB models of low metallicity: the implications for the self-enrichment scenario in metal-poor globular clusters , 2009, 0903.0896.
[53] F. Grundahl,et al. A LARGE C+N+O ABUNDANCE SPREAD IN GIANT STARS OF THE GLOBULAR CLUSTER NGC 1851 , 2009, 0902.1773.
[54] S. Cristallo,et al. Evolution, nucleosynthesis and yields of low mass AGB stars , 2009, 0902.0243.
[55] N. Mowlavi,et al. CNONa and 12 C/ 13 C in giant stars of 10 open clusters ⋆ , 2008, 0810.1701.
[56] A. Renzini. Origin of multiple stellar populations in globular clusters and their helium enrichment , 2008, 0808.4095.
[57] P. Ventura,et al. The self-enrichment scenario in intermediate metallicity globular clusters , 2007, 0712.0247.
[58] Belgium,et al. Evolution of asymptotic giant branch stars. II. Optical to far-infrared isochrones with improved TP- , 2007, 0711.4922.
[59] L. Girardi,et al. THE ACS NEARBY GALAXY SURVEY TREASURY , 2007, 0905.3737.
[60] J. Lattanzio,et al. Stellar Models and Yields of Asymptotic Giant Branch Stars , 2007, Publications of the Astronomical Society of Australia.
[61] Astronomy,et al. Light nuclei in galactic globular clusters: constraints on the self-enrichment scenario from nucleosynthesis , 2007, 0704.3331.
[62] -INAF,et al. Evolution of asymptotic giant branch stars. I. Updated synthetic TP-AGB models and their basic calibration , 2007, astro-ph/0703139.
[63] R. Izzard,et al. Reaction rate uncertainties and the operation of the NeNa and MgAl chains during HBB in intermediate-mass AGB stars , 2007, astro-ph/0703078.
[64] G. Meynet,et al. Fast rotating massive stars and the origin of the abundance patterns in galactic globular clusters , 2006, astro-ph/0611379.
[65] D. A. García-Hernández,et al. Rubidium-Rich Asymptotic Giant Branch Stars , 2006, Science.
[66] P. Ventura,et al. Does the oxygen-sodium anticorrelation in globular clusters require a lowering of the $\mathsf{^{23}}$Na(p,$\mathsf{\alpha)^{20}}$Ne reaction rate? , 2006 .
[67] J. Lattanzio,et al. The Chemical Evolution of Helium in Globular Clusters: Implications for the Self-Pollution Scenario , 2006, astro-ph/0608366.
[68] P. Ventura,et al. Toward a Working Model for the Abundance Variations in Stars within Globular Clusters , 2005, astro-ph/0511603.
[69] M. Cuntz,et al. A New Version of Reimers’ Law of Mass Loss Based on a Physical Approach , 2005, astro-ph/0507598.
[70] P. D’Antona. Full computation of massive AGB evolution. II. The role of mass loss and cross-sections , 2005, astro-ph/0505221.
[71] P. Ventura,et al. Towards a working model for the abundance variations within globular cluster stars , 2005, Proceedings of the International Astronomical Union.
[72] S. Lucatello,et al. Abundances of C, N, O in slightly evolved stars in the globular clusters NGC 6397, NGC 6752 and 47 Tuc , 2004, astro-ph/0411241.
[73] P. Ventura,et al. Full computation of massive AGB evolution. I. The large impact of convection on nucleosynthesis , 2004, astro-ph/0411191.
[74] C. Iliadis,et al. Investigation of the Na-23(p, gamma) Mg-24 and Na-23(p, alpha) Ne-20 reactions via (He-3, d) spectroscopy , 2004 .
[75] J. José,et al. Does an NeNa Cycle Exist in Explosive Hydrogen Burning? , 2004 .
[76] S. Goriely,et al. S-process in hot AGB stars: A complex interplay between diffusive mixing and nuclear burning , 2004 .
[77] J. Lattanzio,et al. Modelling self-pollution of globular clusters from AGB stars , 2004, astro-ph/0406360.
[78] F. Herwig. Dredge-up and Envelope Burning in Intermediate-Mass Giants of Very Low Metallicity , 2003, astro-ph/0312616.
[79] J. Lattanzio,et al. AGB Stars and the Observed Abundance of Neon in Planetary Nebulae , 2003, Publications of the Astronomical Society of Australia.
[80] F. Herwig,et al. The Abundance Evolution of Oxygen, Sodium, and Magnesium in Extremely Metal Poor Intermediate-Mass Stars: Implications for the Self-Pollution Scenario in Globular Clusters , 2003, astro-ph/0305494.
[81] L. Girardi,et al. The red tail of carbon stars in the LMC: Models meet 2MASS and DENIS observations , 2003, astro-ph/0302601.
[82] J. Lattanzio,et al. Parameterising the Third Dredge-up in Asymptotic Giant Branch Stars , 2002, Publications of the Astronomical Society of Australia.
[83] F. Thielemann,et al. Astrophysical reaction rates from statistical model calculations , 2000, astro-ph/0004059.
[84] P. Marigo. Chemical Yields from Low- and Intermediate-Mass Stars , 1999, astro-ph/0012181.
[85] P. Aguer,et al. A compilation of charged-particle induced thermonuclear reaction rates , 1999 .
[86] V. Smith,et al. Star-to-Star Abundance Variations among Bright Giants in the Mildly Metal-poor Globular Cluster M4 , 1999, astro-ph/9905370.
[87] J. Lattanzio,et al. On the Numerical Treatment and Dependence of the Third Dredge-up Phenomenon , 1996 .
[88] C. Charbonnel,et al. Nucleosynthesis of light elements inside thermally pulsing AGB stars - I. The case of intermediate-mass stars , 1996, astro-ph/9608153.
[89] G. Wasserburg,et al. Hot bottom burning in asymptotic giant branch stars and its effect on oxygen isotopic abundances , 1995 .
[90] R. Kurucz. Solar abundance model atmospheres for 0,1,2,4,8 km/s. , 1994 .
[91] P. Wood,et al. Evolution of Low- and Intermediate-Mass Stars to the End of the Asymptotic Giant Branch with Mass Loss , 1993 .
[92] A. I. Boothroyd,et al. Low-Mass Stars. III. Low-Mass Stars with Steady Mass Loss: Up to the Asymptotic Giant Branch and through the Final Thermal Pulses , 1988 .
[93] W. Rodney,et al. Cauldrons in the cosmos , 1988 .