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Results 1 - 3 of 3

Observational constraints on the origin of the elements. VIII. Constraining the Barium, Strontium and Yttrium chemical evolution in metal-poor stars. (arXiv:2311.05459v1 [astro-ph.SR])
- Volume 18, Issue 44 - article #5
- G. Guiglion, M. Bergemann, N. Storm, J. Lian, G. Cescutti, A. Serenelli
- http://arxiv.org/abs/2311.05459
How Many Components? Quantifying the Complexity of the Metallicity Distribution in the Milky Way Bulge with APOGEE. (arXiv:2007.13967v1 [astro-ph.GA])
- Volume 15, Issue 31 - article #6
- A. Rojas-Arriagada, G. Zasowski, M. Schultheis, M. Zoccali, S. Hasselquist, C. Chiappini, R. E. Cohen, K. Cunha, J. G. Fernández-Trincado, F. Fragkoudi, D. A. García-Hernández, D. Geisler, J. Lian, S. Majewski, D. Minniti, C. Nitschelm, A. B. A. Queiroz
- http://arxiv.org/abs/2007.13967
Stellar population models based on the SDSS-IV MaStar library of stellar spectra. I. Intermediate-age/old models. (arXiv:1911.05748v1 [astro-ph.SR])
- Volume 14, Issue 46 - article #7
- C. Maraston, L. Hill, D. Thomas, R. Yan, Y. Chen, J. Lian, T. Parikh, S. Meneses-Goytia, M. Bershady, N. Drory, D. Bizyaev, A. Concas, J. Brownstein, D. Lazarz, G. Stringfellow, K. Stassun
- http://arxiv.org/abs/1911.05748

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