activity
19982026
most citedNeutron capture in low mass Asymptotic Giant Branch stars: cross sections and abundance signatures

927 citations · 6.5k across the 139 of their papers we have counts for

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29 papers · 1 filter

astro-ph2008★ 42 cited

The Role of Massive Agb Stars in the Early Solar System Composition

Josep M. Trigo-Rodriguez, Domingo Anibal Garcia-Hernandez, Maria Lugaro +4

We demonstrate that a massive asymptotic giant branch (AGB) star is a good candidate as the main source of short-lived radionuclides in the early solar system. Recent identificatio…

astro-ph2008

The impact of the 18F(a,p)21Ne reaction on fluorine production in AGB stars

Amanda I. Karakas, Hye Young Lee, Maria Lugaro +2

The recent experimental evaluation of the 18F(a,p)21Ne reaction rate, when considering its associated uncertainties, presented significant differences compared to the theoretical H…

astro-ph2008★ 117 cited

Nucleosynthesis Predictions for Intermediate-Mass AGB Stars: Comparison to Observations of Type I Planetary Nebulae

Amanda I. Karakas, Mark A. van Raai, Maria Lugaro +2

Type I planetary nebulae (PNe) have high He/H and N/O ratios and are thought to be descendants of stars with initial masses of ~3-8Msun. These characteristics indicate that the pro…

astro-ph2008★ 4 cited

Modelling the evolution and nucleosynthesis of carbon-enhanced metal-poor stars

O. R. Pols, R. G. Izzard, M. Lugaro +1

We present the results of binary population simulations of carbon-enhanced metal-poor (CEMP) stars. We show that nitrogen and fluorine are useful tracers of the origin of CEMP star…

astro-ph2008★ 40 cited

Fluorine in carbon-enhanced metal-poor stars: a binary scenario

M. Lugaro, S. E. de Mink, R. G. Izzard +8

A super-solar fluorine abundance was observed in the carbon-enhanced metal-poor (CEMP) star HE 1305+0132 ([F/Fe] = +2.90, [Fe/H] = -2.5). We propose that this observation can be ex…

astro-ph2008★ 55 cited

New reaction rate for 16O(p,gamma)17F and its influence on the oxygen isotopic ratios in massive AGB stars

C. Iliadis, C. Angulo, P. Descouvemont +2

The 16O(p,gamma)17F reaction rate is revisited with special emphasis on the stellar temperature range of T=60-100 MK important for hot bottom burning in asymptotic giant branch (AG…

astro-ph2007★ 25 cited

Reaction rate uncertainties and 26Al in AGB silicon carbide stardust

M. A. van Raai, M. Lugaro, A. I. Karakas +1

Stardust is a class of presolar grains each of which presents an ideally uncontaminated stellar sample. Mainstream silicon carbide (SiC) stardust formed in the extended envelopes o…

astro-ph2007★ 33 cited

The impact of the 18F(a,p)21Ne reaction on asymptotic giant branch nucleosynthesis

Amanda Karakas, Hye Young Lee, Maria Lugaro +2

We present detailed models of low and intermediate-mass asymptotic giant branch (AGB) stars with and without the 18F(a,p)21Ne reaction included in the nuclear network, where the ra…

astro-ph2007★ 18 cited

On the solar abundance of indium

N. Vitas, I. Vince, M. Lugaro +3

The generally adopted value for the solar abundance of indium is over six times higher than the meteoritic value. We address this discrepancy through numerical synthesis of the 451…

astro-ph2007★ 17 cited

Stellar population synthesis of post-AGB stars: the s-process in MACHO47.2496.8

A. Bonacic Marinovic, M. Lugaro, M. Reyniers +1

The low-metallicity RV Tauri star MACHO47.2496.8, recently discovered in the Large Magellanic Cloud, is highly enriched in carbon and heavy elements produced by the slow neutron ca…

astro-ph2007★ 94 cited

Reaction rate uncertainties and the operation of the NeNa and MgAl chains during HBB in intermediate-mass AGB stars

R. G. Izzard, M. Lugaro, A. I. Karakas +2

We test the effect of proton-capture reaction rate uncertainties on the abundances of the Ne, Na, Mg and Al isotopes processed by the NeNa and MgAl chains during hot bottom burning…

astro-ph2007★ 28 cited

Germanium Production in Asymptotic Giant Branch stars: Implications for Observations of Planetary Nebulae

Amanda Karakas, Maria Lugaro, Roberto Gallino

Observations of planetary nebulae (PNe) by Sterling, Dinerstein and Bowers have revealed abundances in the neutron-capture element Germanium (Ge) from solar to factors of 3 -- 10 a…

astro-ph2006★ 35 cited

On the asymptotic giant branch star origin of peculiar spinel grain OC2

M. Lugaro, A. I. Karakas, L. R. Nittler +4

Microscopic presolar grains extracted from primitive meteorites have extremely anomalous isotopic compositions revealing the stellar origin of these grains. The composition of pres…

astro-ph2006★ 2 cited

Population synthesis of s-process element enhanced stars: Constraining the 13C efficiency

A. Bonacic Marinovic, R. G. Izzard, M. Lugaro +1

We study s-process element abundance ratios in stars by carrying out stellar population synthesis, using a rapid synthetic stellar evolution code which includes an up-to-date treat…

astro-ph2006★ 55 cited

Cosmological implications of dwarf spheroidal chemical evolution

Yeshe Fenner, Brad K. Gibson, Roberto Gallino +1

The chemical properties of dwarf spheroidals in the local group are shown to be inconsistent with star formation being truncated after the reionization epoch (z~8). Enhanced levels…

astro-ph2006★ 106 cited

The Uncertainties in the 22Ne + alpha-capture Reaction Rates and the Production of the Heavy Magnesium Isotopes in Asymptotic Giant Branch Stars of Intermediate Mass

A. Karakas, M. Lugaro, M. Wiescher +2

We present new rates for the 22Ne(alpha, n)25Mg and 22Ne(alpha,gamma)26Mg reactions, with uncertainties that have been considerably reduced compared to previous estimates, and we s…

astro-ph2005★ 20 cited

What we do and do not know about the s-process

J. C. Lattanzio, M. A. Lugaro

AGB stars are the source for the main component of the -process. Here we discuss both the properties which are reasonably well known and those which still suffer from substantia…

astro-ph2005★ 37 cited

The effect of the 19F(alpha,p)22Ne reaction rate uncertainty on the yield of fluorine from Wolf-Rayet Stars

R. J. Stancliffe, M. Lugaro, C. Ugalde +3

In the light of recent recalculations of the \el{19}{F}(alpha,p)\el{22}{Ne} reaction rate we present results of the expected yield of \el{19}{F} from Wolf-Rayet (WR) stars. We have…

astro-ph2004★ 3 cited

Constraints on AGB models from the heavy-element composition of presolar SiC grains

M. Lugaro, A. M. Davis, R. Gallino +2

Presolar SiC grains formed around Asymptotic Giant Branch (AGB) stars during their carbon-rich phase and contain heavy elements in trace amounts showing the signature of the slow n…

astro-ph2004★ 5 cited

HR4049: signature of nova nucleosynthesis ?

Maria Lugaro, Onno Pols, Amanda I. Karakas +1

The post-Asymptotic Giant Branch (AGB) star HR4049 is in an eccentric binary system with a relatively short period probably surrounded by a dusty circumbinary disk. Extremely anoma…

astro-ph2004★ 218 cited

Reaction Rates Uncertainties and the Production of F19 in AGB Stars

Maria Lugaro, Claudio Ugalde, Amanda I. Karakas +4

We present nucleosynthesis calculations and the resulting 19F stellar yields for a large set of models with different masses and metallicity. We find that the production of fluorin…

astro-ph2003★ 129 cited

The s-Process in Rotating Asymptotic Giant Branch Stars

Falk Herwig, Norbert Langer, Maria Lugaro

(abridged) We model the nucleosynthesis during the thermal pulse phase of a rotating, solar metallicity AGB star of 3M_sun. Rotationally induced mixing during the thermal pulses pr…

astro-ph2002★ 216 cited

s-Process Nucleosynthesis in AGB Stars: A Test for Stellar Evolution

Maria Lugaro, Falk Herwig, John C. Lattanzio +2

[abridged] We study the s-process in AGB stars using three different stellar evolutionary models computed for a 3Msun and solar metallicity star. First we investigate the formation…

astro-ph2002★ 1 cited

Could SiC A+B grains have originated in a post-AGB thermal pulse?

Falk Herwig, Sachiko Amari, Maria Lugaro +1

The carbon and nitrogen isotopic ratios of pre-solar SiC grains of type A+B suggest a proton-limited nucleosynthetic process as encountered, for instance, during the very late ther…