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pro vyhledávání: '"Bridget L. Ratcliffe"'
Autor:
Bridget L. Ratcliffe, Melissa K. Ness
Publikováno v:
The Astrophysical Journal, Vol 943, Iss 2, p 92 (2023)
Chemical abundances of Milky Way disk stars are empirical tracers of its enrichment history. However, they capture joint-information that is valuable to disentangle. In this work, we quantify how individual abundances evolve across the present-day Ga
Externí odkaz:
https://doaj.org/article/0e7cfb3d7fa14d64ae1f1840667669b3
Autor:
Bridget L. Ratcliffe, Melissa K. Ness, Tobias Buck, Kathryn V. Johnston, Bodhisattva Sen, Leandro Beraldo e Silva, Victor P. Debattista
To understand the formation and evolution of the Milky Way disk, we must connect its current properties to its past. We explore hydrodynamical cosmological simulations to investigate how the chemical abundances of stars might be linked to their origi
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::436adfa198719d5a6f3863c12bd7016a
Publikováno v:
The Astrophysical Journal. 900:165
A major goal in the field of galaxy formation is to understand the formation of the Milky Way’s disk. The first step toward doing this is to empirically describe its present state. We use the new high-dimensional data set of 19 abundances from 27,1
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::ba1451a496a8400cc20ef25d3bfadd86
https://doi.org/10.3847/1538-4357/abac61
https://doi.org/10.3847/1538-4357/abac61