The GOTHAM survey: chemical evolution of Milky Way globular clusters

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Bibliographische Detailangaben
Veröffentlicht in:International Astronomical Union (334. : 2017 : Potsdam) Rediscovering our galaxy
1. Verfasser: Dias, B. (VerfasserIn)
Weitere Verfasser: Barbuy, B. (VerfasserIn), Saviane, I. (VerfasserIn), Held, E. V. (VerfasserIn), Costa, G. Da (VerfasserIn), Ortolani, S. (VerfasserIn), Gullieuszik, M. (VerfasserIn)
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Sprache:eng
Veröffentlicht: 2018
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The oldest stars of the bulge: new information on the ancient Galaxy 2018 Cescutti, G.
Galactic Archeology with RAVE and TGAS 2018 Steinmetz, M.
Massive stars: stellar models and stellar yields, impact on Galactic Archaeology 2018 Meynet, G.
Galactic Phylogenetics 2018 Jofré, P.
Can we really use chemical properties of red-giant stars as age indicators ? 2018 Lagarde, N.
Abundance Analysis for Extremely Metal-Poor Stars from SDSS/SEGUE 2018 Matsuno, T.
The ages of (the oldest) stars 2018 Catelan, M.
Stellar Substructure in the Halos of the Milky Way and M31 2018 Ferguson, A. M. N.
Constraining the Formation and Mass of the Milky Way Halo using Globular Cluster Orbits from HST Proper Motions 2018 Sohn, S. T.
Efficiency and success rates of the Pristine survey from spectroscopic follow-up 2018 Youakim, K.
Large-Scale Surveys of Pulsating Stars for Studying Stellar Populations in the Inner Galaxy 2018 Matsunaga, N.
The APOSTLE simulations: Rotation curves derived from synthetic 21-cm observations 2018 Oman, K. A.
Galactic Archeology with 4MO 2018 Felizing, S.
Closing remarks and Outlook 2018 Combes, F.
The CORAVEL Radial Velocity Data Base 2018 Udry, S.
Study of the thick disc of the Milky Way from a population synthesis model 2018 Nasello, G.
Measurement of [Fe/H] and [C/Fe] for Metal-Poor Stars from the RAVE Survey 2018 Rasmussen, K. C.
Precise distances to red giant stars with seismic data using the near-IR surfacebrightness relation 2018 Storm, J.
Developing an astrophysical line list for Keck/Nirspec observations of red giants in the Galactic centre 2018 Thorsbro, B.
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