Article
Astronomy & Astrophysics
Umberto Battino, Claudia Lederer-Woods, Marco Pignatari, Benjamin Soos, Maria Lugaro, Diego Vescovi, Sergio Cristallo, Philip J. Woods, Amanda Karakas
Summary: This study re-evaluates the production of Al-26 and its impact on stellar nucleosynthesis. The new reactivities have a significant effect on both low- and high-mass stars.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
(2023)
Article
Astronomy & Astrophysics
M. P. Roriz, M. Lugaro, C. B. Pereira, N. A. Drake, S. Junqueira, C. Sneden
Summary: Barium (Ba) stars show atmospheric signs of the slow neutron-capture mechanism from asymptotic giant branch (AGB) stars, with rubidium (Rb) playing a key role in the s-process diagnostic. The study of 180 Ba stars reveals that Rb abundances are consistent with s-process models from low-mass AGB stars, indicating the main neutron source is the C-13(alpha,n)O-16 reaction in the companions of these Ba stars. Former IR/OH massive AGB star companions were not found in this study.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
(2021)
Article
Astronomy & Astrophysics
M. P. Roriz, M. Lugaro, C. B. Pereira, C. Sneden, S. Junqueira, A. Karakas, N. A. Drake
Summary: A new study presents elemental abundances for neutron-capture elements in 180 barium giant stars, revealing discrepancies in La abundances compared to previous literature. The data set shows an overabundance of neutron-capture elements in these stars, but behaves similarly to field stars in some aspects. While model predictions match observations in certain ratios, discrepancies are found in other ratios, requiring further investigation into neutron capture models.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
(2021)
Article
Astronomy & Astrophysics
C. Abia, P. de Laverny, S. Korotin, A. Asensio Ramos, A. Recio-Blanco, N. Prantzos
Summary: By analyzing the Rb and Zr abundances in KM-type giant stars, it was found that there is a Rb deficiency in giant stars, but once NLTE corrections are performed, the ratios are very close to solar values. This contrasts with the Rb deficiency found in M dwarfs, indicating potential differences in nucleosynthesis mechanisms for different types of stars.
ASTRONOMY & ASTROPHYSICS
(2021)
Article
Astronomy & Astrophysics
D. A. Baiko
Summary: This study focuses on the nuclear fusion reactions in white dwarfs and neutron stars, and calculates the plasma screening factor from first principles. It finds good agreement with earlier results and identifies a deviation in reaction rates that can be approximated by a simple analytic expression. The method developed in this study can be extended to ion mixtures and crystallized phases of stellar matter.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
(2021)
Article
Astronomy & Astrophysics
Ben T. Pepper, A. G. Istrate, A. D. Romero, S. O. Kepler
Summary: One of the largest uncertainties in stellar evolutionary computations is the accuracy of the considered reaction rates. This study investigates the impact of uncertainties in the C-12(alpha, gamma)O-16 reaction rates on the evolution of white dwarfs and their progenitors. The results show that the considered reaction rates have significant effects on various stages of stellar evolution.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
(2022)
Article
Astronomy & Astrophysics
Thomas Lawson, Marco Pignatari, Richard J. Stancliffe, Jacqueline den Hartogh, Sam Jones, Chris L. Fryer, Brad K. Gibson, Maria Lugaro
Summary: This study examines the impact of core-collapse supernovae on the production of short-lived radioactive isotopes and finds that explosion energy and remnant mass play crucial roles in determining the final yields of these isotopes.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
(2022)
Article
Astronomy & Astrophysics
Jordan Schofield, Marco Pignatari, Richard J. Stancliffe, Peter Hoppe
Summary: In this study, isotopic abundances of C, N, Al, Si, and Ti measured in presolar grains were compared with predictions from 21 CCSN models. The research found that high energy models favor the formation of a C/Si zone enriched in C-12, Si-28, and Ti-44.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
(2022)
Article
Astronomy & Astrophysics
L. Cavallo, G. Cescutti, F. Matteucci
Summary: In this paper, the authors investigate the origin of the large star-to-star variation in the [Eu/Fe] ratios in extremely metal-poor stars. By considering the chemical enrichment of Eu in the building blocks of the Galactic halo, they find that the dynamics of binary systems in the gravitational potential of the host galaxy play a role in the enrichment from neutron star mergers.
ASTRONOMY & ASTROPHYSICS
(2023)
Article
Astronomy & Astrophysics
Maren Brauner, Thomas Masseron, Domingo A. Garcia-Hernandez, Marco Pignatari, Kate A. Womack, Maria Lugaro, Christian R. Hayes
Summary: The origin of phosphorus, an essential element for life on Earth, is currently unknown. The discovery of phosphorus-rich and metal-poor giants challenges current theories on stellar nucleosynthesis and calls for a search of their progenitor or polluter. By studying a larger sample of phosphorus-rich stars, researchers aim to find a reliable chemical abundance pattern that defines these peculiar stars and contribute to the search for the source of phosphorus in our Galaxy.
ASTRONOMY & ASTROPHYSICS
(2023)
Article
Astronomy & Astrophysics
A. Choplin, S. Goriely, R. Hirschi, N. Tominaga, G. Meynet
Summary: The study investigates the mechanism of p-process nucleosynthesis in rotating massive stars and finds that rotation has a comparable impact on the p-process as on the s-process. The contribution of core-collapse supernovae from massive stars to the solar p-nuclei may have been underestimated in the past.
ASTRONOMY & ASTROPHYSICS
(2022)
Article
Astronomy & Astrophysics
Pavel A. Denissenkov, Falk Herwig, Georgios Perdikakis, Hendrik Schatz
Summary: This study investigates the impact of (n,gamma) reaction rate uncertainties on the predicted abundances of neutron-capture elements in carbon-enhanced metal-poor stars, finding that certain reactions have significant effects on the predicted abundances of barium and praseodymium.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
(2021)
Article
Astronomy & Astrophysics
Pavel A. Denissenkov, Chris Ruiz, Sriteja Upadhyayula, Falk Herwig
Summary: Recent spectroscopic measurements reveal high abundances of Be-7 in nova ejecta, deviating from theoretical predictions, but the assumption of enhanced He-4 abundances helps reduce this discrepancy.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
(2021)
Article
Astronomy & Astrophysics
E. Monpribat, S. Martinet, S. Courtin, M. Heine, S. Ekstrom, D. G. Jenkins, A. Choplin, P. Adsley, D. Curien, M. Moukaddam, J. Nippert, S. Tsiatsiou, G. Meynet
Summary: This study provides new numerical tables for C-12 + C-12 reaction rates and associated uncertainty estimations, along with analytical formulae that can be directly implemented into stellar evolution codes. The impact of these new rates on C-burning in stars was investigated, showing differences in central temperatures and burning lifetimes.
ASTRONOMY & ASTROPHYSICS
(2022)
Article
Astronomy & Astrophysics
M. Deal, C. J. A. P. Martins
Summary: The success of primordial nucleosynthesis has been limited by the long-standing lithium problem. A self-consistent perturbative analysis is used to explore the problem and its possible solutions in the context of the latest observations and theoretical modeling. The research concludes that the lithium problem most likely has an astrophysical solution, while the Deuterium discrepancy provides a possible indication of new physics.
ASTRONOMY & ASTROPHYSICS
(2021)
Article
Astronomy & Astrophysics
Michael Hanke, Camilla Juul Hansen, Hans-Guenter Ludwig, Sergio Cristallo, Andrew McWilliam, Eva K. Grebel, Luciano Piersanti
ASTRONOMY & ASTROPHYSICS
(2020)
Article
Astronomy & Astrophysics
A. Skuladottir, C. J. Hansen, A. Choplin, S. Salvadori, M. Hampel, S. W. Campbell
ASTRONOMY & ASTROPHYSICS
(2020)
Article
Astronomy & Astrophysics
F. Primas
Article
Astronomy & Astrophysics
R. Theler, P. Jablonka, R. Lucchesi, C. Lardo, P. North, M. Irwin, G. Battaglia, V. Hill, E. Tolstoy, K. Venn, A. Helmi, A. Kaufer, F. Primas, M. Shetrone
ASTRONOMY & ASTROPHYSICS
(2020)
Article
Astronomy & Astrophysics
L. Sbordone, C. J. Hansen, L. Monaco, S. Cristallo, P. Bonifacio, E. Caffau, S. Villanova, P. Amigo
ASTRONOMY & ASTROPHYSICS
(2020)
Article
Astronomy & Astrophysics
M. Reichert, C. J. Hansen, M. Hanke, A. Skuladottir, A. Arcones, E. K. Grebel
ASTRONOMY & ASTROPHYSICS
(2020)
Article
Astronomy & Astrophysics
R. Lucchesi, C. Lardo, F. Primas, P. Jablonka, P. North, G. Battaglia, E. Starkenburg, V. Hill, M. Irwin, P. Francois, M. Shetrone, E. Tolstoy, K. Venn
ASTRONOMY & ASTROPHYSICS
(2020)
Article
Astronomy & Astrophysics
C. J. Hansen, A. Koch, L. Mashonkina, M. Magg, M. Bergemann, T. Sitnova, A. J. Gallagher, I. Ilyin, E. Caffau, H. W. Zhang, K. G. Strassmeier, R. S. Klessen
ASTRONOMY & ASTROPHYSICS
(2020)
Article
Astronomy & Astrophysics
Andreas J. Koch-Hansen, Camilla Juul Hansen, Linda Lombardo, Piercarlo Bonifacio, Michael Hanke, Elisabetta Caffau
Summary: The paper presents a detailed chemical abundance analysis of the halo star J110842, previously kinematically associated with the massive MW GC omega Centauri. The star's metallicity and abundance distributions are closely compatible with omega Centauri, suggesting a possible origin as a second-generation GC star. However, its overlap with other MW components complicates a clear-cut distinction of its origin.
ASTRONOMY & ASTROPHYSICS
(2021)
Article
Astronomy & Astrophysics
M. Reichert, C. J. Hansen, A. Arcones
Summary: This study presents three r-process enhanced stars in the dwarf spheroidal galaxy Fornax, with extreme Eu enrichment and high metallicities. The discovery of these stars opens up new opportunities to understand the origin of heavy elements formed by the r-process.
ASTROPHYSICAL JOURNAL
(2021)
Article
Astronomy & Astrophysics
Dongwook Lim, Andreas J. Koch-Hansen, Camilla Juul Hansen, Sebastien Lepine, Jennifer L. Marshall, Mark Wilkinson, Jorge Penarrubia
Summary: Recent discoveries of wide binaries have shed light on their chemical compositions and potential origins, with some possibly forming in dwarf galaxy environments with lower metallicities. Further research provides a novel opportunity to understand the formation of wide binaries and the assembly process of the Milky Way.
ASTRONOMY & ASTROPHYSICS
(2021)
Article
Astronomy & Astrophysics
Camilla Juul Hansen
Summary: The formation of heavy elements is a long-standing question in physics. Recent studies have provided evidence of nuclear processes and heavy element behavior in evolved stars. However, the conditions of neutron-capture reactions are poorly understood and require a multidisciplinary effort to improve our understanding. Detailed observations in the near-UV to blue wavelength region are crucial, and the development of new instruments can enhance the quality and signal-to-noise ratio of observations.
EXPERIMENTAL ASTRONOMY
(2023)
Article
Astronomy & Astrophysics
A. Psaltis, A. Arcones, F. Montes, P. Mohr, C. J. Hansen, M. Jacobi, H. Schatz
Summary: This study investigates the impact of nuclear reactions on the synthesis of lighter heavy elements. Using a Monte Carlo approach and improved (alpha, xn) rates, the study identifies the effects of (alpha, xn) reaction rates on elemental ratios in different astrophysical conditions. The study calls for more nuclear physics experiments and observational studies of metal-poor stars.
ASTROPHYSICAL JOURNAL
(2022)
Article
Astronomy & Astrophysics
Gustavo E. Medina, Camilla J. Hansen, Ricardo R. Munoz, Eva K. Grebel, A. Katherina Vivas, Jeffrey L. Carlin, Clara E. Martinez-Vazquez
Summary: We conducted spectroscopic analysis of 20 halo ab-type RR Lyrae stars using medium-resolution spectra, obtaining systemic velocities of targets with uncertainties of 5-10 km s(-1) and calculating orbital parameters for a subsample. Our findings suggest that at least half of the sample stars might have an accreted origin, based on their orbital orientations in an isolated Milky Way or a perturbed model by the Large Magellanic Cloud. We also derived atmospheric parameters and chemical abundance ratios for seven stars beyond 20 kpc, with some displaying underabundance of alpha-elements, indicating association with accretion events.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
(2023)
Article
Astronomy & Astrophysics
Daniela Carollo, Masashi Chiba, Miho Ishigaki, Ken Freeman, Timothy C. Beers, Young Sun Lee, Patricia Tissera, Chiara Battistini, Francesca Primas
ASTROPHYSICAL JOURNAL
(2019)