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investigation of Stars In the Milky way with Bayesian statistics and Asteroseismology

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Month: August 2020

Papers

Chemical evolution of the Milky Way: constraints on the formation of the thick and thin discs

Marco Palla, Francesca Matteucci, Emanuele Spitoni, Fiorenzo Vincenzo, Valeria Grisoni

Chemical evolution of the Milky Way: constraints on the formation of the thick and thin discs
See arXiv version
18 pages, 12 figures, 5 tables. Accepted for publication in MNRAS

Continue reading “Chemical evolution of the Milky Way: constraints on the formation of the thick and thin discs” →

August 17, 2020September 7, 2020emanueleLeave a comment
Papers

Fluorine in the solar neighborhood: modelling the Galactic thick and thin discs

Valeria Grisoni, Donatella Romano, Emanuele Spitoni, Francesca Matteucci, Nils Ryde, Henrik Jönsson

Fluorine in the solar neighborhood: modelling the Galactic thick and thin discs
See arXiv version
8 pages, 2 figures. Accepted for publication in MNRAS

Continue reading “Fluorine in the solar neighborhood: modelling the Galactic thick and thin discs” →

August 3, 2020September 7, 2020emanueleLeave a comment
Announcements

Mark L. Winther joins iSIMBA

Mark L. Winther joins SAC and the iSIMBA group as a PhD student on 1 August 2020.

Mark will be working on improving models of stellar evolution for solar-like oscillators and especially on improving 3D hydrodynamical simulations of stellar atmospheres.

Read more about Mark and the rest of the group here: People

August 1, 2020September 7, 2020Leave a comment

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Recent

  • Scaling relations of convective granulation noise across the HR diagram from 3D stellar atmosphere models
  • Disc dichotomy signature in the vertical distribution of [Mg/Fe] and the delayed gas infall scenario
  • The Seventeenth Data Release of the Sloan Digital Sky Surveys: Complete Release of MaNGA, MaStar and APOGEE-2 Data
  • Chemo-dynamics and asteroseismic ages of seven metal-poor red giants from the Kepler field
  • The SAPP pipeline for the determination of stellar abundances and atmospheric parameters of stars in the core program of the PLATO mission

News

  • Scaling relations of convective granulation noise across the HR diagram from 3D stellar atmosphere models
  • Disc dichotomy signature in the vertical distribution of [Mg/Fe] and the delayed gas infall scenario
  • The Seventeenth Data Release of the Sloan Digital Sky Surveys: Complete Release of MaNGA, MaStar and APOGEE-2 Data
  • Chemo-dynamics and asteroseismic ages of seven metal-poor red giants from the Kepler field
  • The SAPP pipeline for the determination of stellar abundances and atmospheric parameters of stars in the core program of the PLATO mission

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iSIMBA @ SAC @ Aarhus University

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