APOGEE DR14/DR15 Abundances in the Inner Milky Way

G. Zasowski, M. Schultheis, S. Hasselquist, K. Cunha, J. Sobeck, J. A. Johnson, A. Rojas-Arriagada, S. R. Majewski, B. H. Andrews, H. Jönsson, T. C. Beers, S. D. Chojnowski, P. M. Frinchaboy, J. A. Holtzman, D. Minniti, D. L. Nidever, C. Nitschelm

Resultado de la investigación: Article

4 Citas (Scopus)

Resumen

We present an overview of the distributions of 11 elemental abundances in the Milky Way's (MW) inner regions, as traced by APOGEE stars released as part of the Sloan Digital Sky Survey Data Release 14/15 (DR14/DR15), including O, Mg, Si, Ca, Cr, Mn, Co, Ni, Na, Al, and K. This sample spans ∼4000 stars with R GC ≤ 4.0 kpc, enabling the most comprehensive study to date of these abundances and their variations within the innermost few kiloparsecs of the MW. We describe the observed abundance patterns ([X/Fe]-[Fe/H]), compare to previous literature results and to patterns in stars at the solar Galactocentric radius (R GC ), and discuss possible trends with DR14/DR15 effective temperatures. We find that the position of the [Mg/Fe]-[Fe/H] "knee" is nearly constant with R GC , indicating a well-mixed star-forming medium or high levels of radial migration in the early inner Galaxy. We quantify the linear correlation between pairs of elements in different subsamples of stars and find that these relationships vary; some abundance correlations are very similar between the α-rich and α-poor stars, but others differ significantly, suggesting variations in the metallicity dependencies of certain supernova yields. These empirical trends will form the basis for more detailed future explorations and for the refinement of model comparison metrics. That the inner MW abundances appear dominated by a single chemical evolutionary track and that they extend to such high metallicities underscore the unique importance of this part of the Galaxy for constraining the ingredients of chemical evolution modeling and for improving our understanding of the evolution of the Galaxy as a whole.

Idioma originalEnglish
Número de artículo138
PublicaciónAstrophysical Journal
Volumen870
N.º2
DOI
EstadoPublished - 10 ene 2019

Huella dactilar

stars
galaxies
metallicity
trends
chemical evolution
ingredients
supernovae
radii
modeling
temperature
chemical
trend

ASJC Scopus subject areas

  • Astronomy and Astrophysics
  • Space and Planetary Science

Citar esto

Zasowski, G., Schultheis, M., Hasselquist, S., Cunha, K., Sobeck, J., Johnson, J. A., ... Nitschelm, C. (2019). APOGEE DR14/DR15 Abundances in the Inner Milky Way. Astrophysical Journal, 870(2), [138]. https://doi.org/10.3847/1538-4357/aaeff4
Zasowski, G. ; Schultheis, M. ; Hasselquist, S. ; Cunha, K. ; Sobeck, J. ; Johnson, J. A. ; Rojas-Arriagada, A. ; Majewski, S. R. ; Andrews, B. H. ; Jönsson, H. ; Beers, T. C. ; Chojnowski, S. D. ; Frinchaboy, P. M. ; Holtzman, J. A. ; Minniti, D. ; Nidever, D. L. ; Nitschelm, C. / APOGEE DR14/DR15 Abundances in the Inner Milky Way. En: Astrophysical Journal. 2019 ; Vol. 870, N.º 2.
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Zasowski, G, Schultheis, M, Hasselquist, S, Cunha, K, Sobeck, J, Johnson, JA, Rojas-Arriagada, A, Majewski, SR, Andrews, BH, Jönsson, H, Beers, TC, Chojnowski, SD, Frinchaboy, PM, Holtzman, JA, Minniti, D, Nidever, DL & Nitschelm, C 2019, 'APOGEE DR14/DR15 Abundances in the Inner Milky Way', Astrophysical Journal, vol. 870, n.º 2, 138. https://doi.org/10.3847/1538-4357/aaeff4

APOGEE DR14/DR15 Abundances in the Inner Milky Way. / Zasowski, G.; Schultheis, M.; Hasselquist, S.; Cunha, K.; Sobeck, J.; Johnson, J. A.; Rojas-Arriagada, A.; Majewski, S. R.; Andrews, B. H.; Jönsson, H.; Beers, T. C.; Chojnowski, S. D.; Frinchaboy, P. M.; Holtzman, J. A.; Minniti, D.; Nidever, D. L.; Nitschelm, C.

En: Astrophysical Journal, Vol. 870, N.º 2, 138, 10.01.2019.

Resultado de la investigación: Article

TY - JOUR

T1 - APOGEE DR14/DR15 Abundances in the Inner Milky Way

AU - Zasowski, G.

AU - Schultheis, M.

AU - Hasselquist, S.

AU - Cunha, K.

AU - Sobeck, J.

AU - Johnson, J. A.

AU - Rojas-Arriagada, A.

AU - Majewski, S. R.

AU - Andrews, B. H.

AU - Jönsson, H.

AU - Beers, T. C.

AU - Chojnowski, S. D.

AU - Frinchaboy, P. M.

AU - Holtzman, J. A.

AU - Minniti, D.

AU - Nidever, D. L.

AU - Nitschelm, C.

PY - 2019/1/10

Y1 - 2019/1/10

N2 - We present an overview of the distributions of 11 elemental abundances in the Milky Way's (MW) inner regions, as traced by APOGEE stars released as part of the Sloan Digital Sky Survey Data Release 14/15 (DR14/DR15), including O, Mg, Si, Ca, Cr, Mn, Co, Ni, Na, Al, and K. This sample spans ∼4000 stars with R GC ≤ 4.0 kpc, enabling the most comprehensive study to date of these abundances and their variations within the innermost few kiloparsecs of the MW. We describe the observed abundance patterns ([X/Fe]-[Fe/H]), compare to previous literature results and to patterns in stars at the solar Galactocentric radius (R GC ), and discuss possible trends with DR14/DR15 effective temperatures. We find that the position of the [Mg/Fe]-[Fe/H] "knee" is nearly constant with R GC , indicating a well-mixed star-forming medium or high levels of radial migration in the early inner Galaxy. We quantify the linear correlation between pairs of elements in different subsamples of stars and find that these relationships vary; some abundance correlations are very similar between the α-rich and α-poor stars, but others differ significantly, suggesting variations in the metallicity dependencies of certain supernova yields. These empirical trends will form the basis for more detailed future explorations and for the refinement of model comparison metrics. That the inner MW abundances appear dominated by a single chemical evolutionary track and that they extend to such high metallicities underscore the unique importance of this part of the Galaxy for constraining the ingredients of chemical evolution modeling and for improving our understanding of the evolution of the Galaxy as a whole.

AB - We present an overview of the distributions of 11 elemental abundances in the Milky Way's (MW) inner regions, as traced by APOGEE stars released as part of the Sloan Digital Sky Survey Data Release 14/15 (DR14/DR15), including O, Mg, Si, Ca, Cr, Mn, Co, Ni, Na, Al, and K. This sample spans ∼4000 stars with R GC ≤ 4.0 kpc, enabling the most comprehensive study to date of these abundances and their variations within the innermost few kiloparsecs of the MW. We describe the observed abundance patterns ([X/Fe]-[Fe/H]), compare to previous literature results and to patterns in stars at the solar Galactocentric radius (R GC ), and discuss possible trends with DR14/DR15 effective temperatures. We find that the position of the [Mg/Fe]-[Fe/H] "knee" is nearly constant with R GC , indicating a well-mixed star-forming medium or high levels of radial migration in the early inner Galaxy. We quantify the linear correlation between pairs of elements in different subsamples of stars and find that these relationships vary; some abundance correlations are very similar between the α-rich and α-poor stars, but others differ significantly, suggesting variations in the metallicity dependencies of certain supernova yields. These empirical trends will form the basis for more detailed future explorations and for the refinement of model comparison metrics. That the inner MW abundances appear dominated by a single chemical evolutionary track and that they extend to such high metallicities underscore the unique importance of this part of the Galaxy for constraining the ingredients of chemical evolution modeling and for improving our understanding of the evolution of the Galaxy as a whole.

KW - Galaxy: abundances

KW - Galaxy: bulge

KW - stars: abundances

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U2 - 10.3847/1538-4357/aaeff4

DO - 10.3847/1538-4357/aaeff4

M3 - Article

VL - 870

JO - Astrophysical Journal

JF - Astrophysical Journal

SN - 0004-637X

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Zasowski G, Schultheis M, Hasselquist S, Cunha K, Sobeck J, Johnson JA y otros. APOGEE DR14/DR15 Abundances in the Inner Milky Way. Astrophysical Journal. 2019 ene 10;870(2). 138. https://doi.org/10.3847/1538-4357/aaeff4