Using chemical tagging to redefine the interface of the Galactic disc and halo
By K. Hawkins, Paulina Jofré, T. Masseron, G. Gilmore. 2015
135 citations recorded by the source corpus.
We present a chemical abundance distribution study in 14 $\alpha$, odd-Z, even-Z, light, and Fe-peak elements of approximately 3200 intermediate metallicity giant stars from the APOGEE survey. The main aim of our analysis is to explore the Galactic disk-halo transition region between -1.20 $<$ [Fe/H] $<$ -0.55 as a means to study chemical difference (and similarities) between these components. In this paper, we show that there is an $\alpha$-poor and $\alpha$-rich sequence within both the metal-poor and intermediate metallicity regions. Using the Galactic rest-frame radial velocity and spatial positions, we further separate our sample into the canonical Galactic components. We then studied the abundances ratios, of Mg, Ti, Si, Ca, O, S, Al, C+N, Na, Ni, Mn, V, and K for each of the components and found the following: (1) the $\alpha$-poor halo subgroup is chemically distinct in the $\alpha$-elements (particularly O, Mg, and S), Al, C+N, and Ni from the $\alpha$-rich halo, consistent with the literature confirming the existence of an $\alpha$-poor accreted halo population; (2) the canonical thick disk and halo are not chemically distinct in all elements indicating a smooth transition between the thick disk and halo; (3) a subsample of the $\alpha$-poor stars at metallicities as low as [Fe/H] $\sim$ -0.85 dex are chemically and dynamically consistent with the thin disk indicating that the thin disk may extend to lower metallicities than previously thought, and (4) that the location of the most metal-poor thin disk stars are consistent with a negative radial metallicity gradient. Finally, we used our analysis to suggest a new set of chemical abundance planes ([$\alpha$/Fe], [C+N/Fe], [Al/Fe], and [Mg/Mn]) that may be able to chemically label the Galactic components in a clean and efficient way independent of kinematics.
Subfields: Astronomy and Astrophysics, Instrumentation
View Paper: https://www.semanticscholar.org/paper/8547341c3b5aba454d3d0acbc4fdd33ef329722a
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In Astronomy and Astrophysics
- Joss Bland-Hawthorn
- O. Gerhard
- I. Minchev
- Hans-Walter Rix
- P. McMillan
- Y. Ting 丁
- Kenneth C. Freeman
- Martin Asplund
In Instrumentation
- Joss Bland-Hawthorn
- O. Gerhard
- P. McMillan
- Kenneth C. Freeman
- M. Ness
- Geraint F. Lewis
- Sanjib Sharma
- P. Kafle
Citations in the corpus
- The GALAH survey and Gaia DR2: dissecting the stellar disc’s phase space by age, action, chemistry, and location (2018, background): “In recent years, this chemical distinction has been further emphasized by enhanced C/N in the older α-rich population, presumably due to the effects of dredge-up in old turn-off dwarfs and giants (Masseron & Gilmore 2015; Hawkins et al. 2015).”
- The Galaxy in Context: Structural, Kinematic, and Integrated Properties (2016, background): “Hawkins et al. (2015) emphasize that a more expanded chemical (C) space may be called for to ensure that the thick disk can be separated from both the thin disk and the lower halo, i.e., C([α/Fe], [C+N/Fe], [Al/Fe], [Mg/Mn]).”