Article
Astronomy & Astrophysics
A. Hui-Bon-Hoa
Summary: The study focuses on the effects of self-consistent Rosseland mean opacity calculations on stellar structure and evolution, compared with models using fixed metal mixtures. The developed strategy allows fast calculations of Rosseland opacities consistent with the chemical mix in the star. The self-consistent models show minimal structural differences compared to models with fixed metal mixtures.
ASTRONOMY & ASTROPHYSICS
(2021)
Article
Astronomy & Astrophysics
A. Hui-Bon-Hoa, J-C Pain, O. Richard
Summary: This study investigates the impact of newly computed monochromatic cross sections on the Rosseland mean opacity of nickel and on the structure of main-sequence massive pulsators. The results show that the new data has similar Rosseland opacities to the Opacity Project or OPAL at high temperatures, but significant differences are observed at lower temperatures.
ASTRONOMY & ASTROPHYSICS
(2022)
Article
Astronomy & Astrophysics
Yaroslav V. Voronov, Svetlana A. Yakovleva, Andrey K. Belyaev
Summary: This paper investigates the inelastic processes in B + H and B+ + H- collisions, taking into account the fine structure. The calculations show that considering the fine structure can significantly change the rate coefficients, and these rates cannot be obtained by simply redistributing the non-relativistic rates. The processes identified in this study are important for non-local thermodynamic equilibrium modeling of stellar atmospheres.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
(2023)
Article
Astronomy & Astrophysics
I Baraffe, T. Constantino, J. Clarke, A. Le Saux, T. Goffrey, T. Guillet, J. Pratt, D. G. Vlaykov
Summary: Recent simulations suggest that convection flows at the boundary of the convective envelope can modify the thermal background in the overshooting layer. By implementing a simple prescription in stellar evolution codes, researchers are able to reproduce the behavior found in hydrodynamical simulations. The introduction of local heating in the overshooting layer reduces the sound-speed discrepancy between solar models and observations, and also affects key quantities in the convective envelope.
ASTRONOMY & ASTROPHYSICS
(2022)
Article
Astronomy & Astrophysics
E. Marini, C. Ventura, M. Tailo, P. Ventura, F. Dell'Agli, M. Castellani
Summary: By comparing observations with stellar evolution modeling, it is found that there is extra mixing from the core during the main sequence evolution of the binary star α Aurigae. This process is crucial for understanding the core hydrogen and helium burning phases of stars. The age of the system is estimated to be 710 million years and the masses of its stars fall into the range of 2.5 to 2.6 solar masses.
ASTRONOMY & ASTROPHYSICS
(2023)
Article
Astronomy & Astrophysics
W. Li, P. Jonsson, A. M. Amarsi, M. C. Li, J. Grumer
Summary: As the most abundant element in the universe after hydrogen and helium, oxygen plays a crucial role in various astrophysical phenomena. This study provides extensive atomic data for oxygen, including lifetimes and transition probabilities, which are important for abundance analyses. The computed transition rates show high accuracy, with 205 transitions having uncertainties smaller than 10%. The new log(gf) values significantly influence the solar oxygen abundance, suggesting a value of log epsilon(O) = 8.70 +/- 0.04.
ASTRONOMY & ASTROPHYSICS
(2023)
Article
Astronomy & Astrophysics
Liuyan Zhao, Hanfeng Song, Georges Meynet, Andre Maeder, Sylvia Ekstrom, Ruiyu Zhang, Ying Qin, Shitao Qi, Qiong Zhan
Summary: This study mainly investigates the impact of rapid rotation and low metallicity on the formation of the blue loop. The results indicate that both factors tend to restrain the development of the outer convective envelope of stars, which disfavors the occurrence and extension of the blue loop.
ASTRONOMY & ASTROPHYSICS
(2023)
Article
Astronomy & Astrophysics
R. Farmer, M. Renzo, Y. Goetberg, E. Bellinger, S. Justham, S. E. de Mink
Summary: In this study, the researchers calculated the evolutionary models of T.ZOs and predicted their observational properties such as temperature, luminosity, pulsation period, and nucleosynthetic products. The models suggest that T.ZOs can be stable over a larger mass range without a gap in their mass distribution. A new nucleosynthetic signal, involving isotopologues (44) TiO2 and (44) TiO, is proposed to identify T.ZOs. The study also explains the difficulty in finding T.ZOs based on their low heavy metal enrichment in the local Universe.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
(2023)
Article
Astronomy & Astrophysics
C. Chiosi, S. Pasetto, E. Chiosi, D. Crnojevic
Summary: This study re-examines the physical foundations and results of the scale-free theory of stellar convection (SFCT), addresses misconceptions and criticisms, and presents recent improvements. The main results include a detailed discussion of boundary conditions for stability analysis in asteroseismology, a quantitative comparison with the mixing length theory, and the recovery of the mixing length theory as a particular case of the SFCT without the need for the mixing length parameter.
ASTRONOMY & ASTROPHYSICS
(2023)
Article
Astronomy & Astrophysics
Erin R. Higgins, Jorick S. Vink, Raphael Hirschi, Alison M. Laird, Gautham N. Sabhahit
Summary: The most massive stars play a crucial role in providing recycled material for young clusters and galaxies. These stars lose a disproportionately large amount of mass from the beginning of their core H-burning. They also release a significant amount of H-processed elements on the main sequence, which may have implications for observed anticorrelations. The primary source of Al-26 is found to be VMS with enhanced winds, contradicting previous theories.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
(2023)
Article
Astronomy & Astrophysics
T. Dumont, A. Palacios, C. Charbonnel, O. Richard, L. Amard, K. Augustson, S. Mathis
Summary: The study explores the impact of additional transport processes on the evolution of rotating stars, focusing on agreement with observations regarding Li-7 depletion, rotation evolution of solar-type stars, and the solar rotation profile. Penetrative convection is found to be relevant for depletion of Li-7 in pre-main sequence and early main sequence stars, whereas the addition of vertical viscosity enables efficient angular momentum transport between the core and envelope, matching solar rotation profile.
ASTRONOMY & ASTROPHYSICS
(2021)
Article
Astronomy & Astrophysics
Jiaolong Zeng, Yongjun Li, Jianmin Yuan
Summary: This study investigates the impact of plasma-screening on electron impact excitation and ionization cross-sections, effective collision strengths, and rate coefficients in dense plasmas under stellar interior conditions. The results show that plasma screening leads to a decrease in electron impact excitation cross-sections while significantly increasing collision ionization cross-sections.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
(2021)
Article
Astronomy & Astrophysics
T. M. Sitnova, S. A. Yakovleva, A. K. Belyaev, L. Mashonkina
Summary: In this study, a new model atom of Zn i-Zn ii was presented based on the most up-to-date data. The non-LTE abundances of Zn i and Zn ii were analyzed in the UV spectra of two metal-poor stars. It was found that non-LTE significantly affects the abundance of Zn i, while the impact on Zn ii is minor. The abundance of zinc was also determined for a sample of 80 stars, revealing variations with metallicity.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
(2022)
Article
Astronomy & Astrophysics
W. Li, A. M. Amarsi, A. Papoulia, J. Ekman, P. Jonsson
Summary: Accurate atomic data are crucial for opacity calculations and abundance analyses of stars. This work aims to provide precise energy levels and transition data for carbon using advanced computational methods. Extensive comparisons with experimental and theoretical results show good agreement, with average uncertainties estimated for different carbon ions.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
(2021)
Article
Astronomy & Astrophysics
Stephen M. Feeney, Benjamin D. Wandelt, Melissa K. Ness
Summary: Upcoming million-star spectroscopic surveys have the potential to revolutionize our view of the formation and chemical evolution of the Milky Way. The automated approach introduced in SSSpaNG optimizes estimates of stellar properties by inferring model parameters from a sample of red clump stars, pooling information between stars to infer their covariance and identifying correlations between spectral pixels. By harnessing the correlation structure of the spectra, the inferred true spectra of red clump stars show significant improvements in denoising and inpainting missing regions, leading to enhanced chemical elemental abundance estimates for individual stars.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
(2021)