The GALAH survey: properties of the Galactic disc(s) in the solar neighbourhood. Issue 4 (27th February 2018)

• Record Type: Journal Article
• Authors: Duong, L; Freeman, K C; Asplund, M; Casagrande, L; Buder, S; Lind, K; Ness, M; Bland-Hawthorn, J; De Silva, G M; D'Orazi, V; Kos, J; Lewis, G F; Lin, J; Martell, S L; Schlesinger, K; Sharma, S; Simpson, J D; Zucker, D B; Zwitter, T; Anguiano, B; Da Costa, G S; Hyde, E; Horner, J; Kafle, P R; Nataf, D M; Reid, W; Stello, D; Ting, Y-S; Wyse, R F G
• Is Part Of: Monthly notices of the Royal Astronomical Society. Volume 476:Issue 4(2018)
• Page Start: 5216
• Page End: 5232
• Publication Date: 2018-02-27
• Subjects: surveys -- stars: abundances -- Galaxy: disc -- Galaxy: evolution -- Galaxy: formation; Astronomy -- Periodicals; Periodicals; 520.5
• DOI: 10.1093/mnras/sty525
• Languages: English
• ISSNs: 0035-8711

Abstract

Abstract: Using data from the GALAH pilot survey, we determine properties of the Galactic thin and thick discs near the solar neighbourhood. The data cover a small range of Galactocentric radius ($7.9 \lesssim R_\mathrm{GC} \lesssim 9.5$ kpc), but extend up to 4 kpc in height from the Galactic plane, and several kpc in the direction of Galactic anti-rotation (at longitude 260° ≤ ℓ ≤ 280°). This allows us to reliably measure the vertical density and abundance profiles of the chemically and kinematically defined 'thick' and 'thin' discs of the Galaxy. The thin disc (low-α population) exhibits a steep negative vertical metallicity gradient, at d[M/H]/d z = −0.18 ± 0.01 dex kpc −1, which is broadly consistent with previous studies. In contrast, its vertical α-abundance profile is almost flat, with a gradient of d[α/M]/d z = 0.008 ± 0.002 dex kpc −1 . The steep vertical metallicity gradient of the low-α population is in agreement with models where radial migration has a major role in the evolution of the thin disc. The thick disc (high-α population) has a weaker vertical metallicity gradient d[M/H]/d z = −0.058 ± 0.003 dex kpc −1 . The α-abundance of the thick disc is nearly constant with height, d[α/M]/d z = 0.007 ± 0.002 dex kpc −1 . The negative gradient in metallicity and the small gradient in [α/M] indicate that the high-α population experienced a settling phase, but also formed prior to the onset of major Type Ia supernova enrichment. We explore the implications of the distinct α-enrichments and narrow [α/M] range of the sub-populations in the context of thick disc formation.