Search Results - "Magg, Ekaterina"

Metal Mixing in the r-process Enhanced Ultrafaint Dwarf Galaxy Reticulum II by Ji, Alexander P., Simon, Joshua D., Roederer, Ian U., Magg, Ekaterina, Frebel, Anna, Johnson, Christian I., Klessen, Ralf S., Magg, Mattis, Cescutti, Gabriele, Mateo, Mario, Bergemann, Maria, Bailey, John I.

“…The ultrafaint dwarf galaxy Reticulum II was enriched by a single rare and prolific r -process event. The r -process content of Reticulum II thus provides a…”
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Metal Mixing in the r-process Enhanced Ultrafaint Dwarf Galaxy Reticulum II This paper includes data gathered with the 6.5 m Magellan Telescopes, located at Las Campanas Observatory, Chile by Ji, Alexander P., Simon, Joshua D., Roederer, Ian U., Magg, Ekaterina, Frebel, Anna, Johnson, Christian I., Klessen, Ralf S., Magg, Mattis, Cescutti, Gabriele, Mateo, Mario, Bergemann, Maria, Bailey, John I.

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Non-LTE Radiative Transfer with Turbospectrum by Gerber, Jeffrey M, Magg, Ekaterina, Plez, Bertrand, Bergemann, Maria, Heiter, Ulrike, Olander, Terese, Hoppe, Richard

“…A&A 669, A43 (2023) Physically realistic models of stellar spectra are needed in a variety of astronomical studies, from the analysis of fundamental stellar…”
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Metal Mixing in the R-Process Enhanced Ultra-Faint Dwarf Galaxy Reticulum II by Ji, Alexander P, Simon, Joshua D, Roederer, Ian U, Magg, Ekaterina, Frebel, Anna, Johnson, Christian I, Klessen, Ralf S, Magg, Mattis, Cescutti, Gabriele, Mateo, Mario, Bergemann, Maria, BaileyIII, John I

“…The ultra-faint dwarf galaxy Reticulum~II was enriched by a single rare and prolific r-process event. The r-process content of Reticulum~II thus provides a…”
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Observational constraints on the origin of the elements. IV: The standard composition of the Sun by Magg, Ekaterina, Bergemann, Maria, Serenelli, Aldo, Bautista, Manuel, Plez, Bertrand, Heiter, Ulrike, Gerber, Jeffrey M, Ludwig, Hans-Günter, Basu, Sarbani, Ferguson, Jason W, Gallego, Helena Carvajal, Gamrath, Sébastien, Palmeri, Patrick, Quinet, Pascal

“…A&A 661, A140 (2022) The chemical composition of the Sun is requested in the context of various studies in astrophysics, among them in the calculation of the…”
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