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Journal Articles Monthly Notices of the Royal Astronomical Society Year : 2017

Using the multi-object adaptive optics demonstrator RAVEN to observe metal-poor stars in and towards the Galactic Centre

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M. Lamb
  • Function : Author
K. Venn
  • Function : Author
D. Andersen
  • Function : Author
S. Oya
  • Function : Author
M. Shetrone
A. Fattahi
  • Function : Author
L. Howes
  • Function : Author
M. Asplund
  • Function : Author
O. Lardière
  • Function : Author
M. Akiyama
  • Function : Author
Y. Ono
  • Function : Author
H. Terada
  • Function : Author
Y. Hayano
  • Function : Author
G. Suzuki
  • Function : Author
C. Blain
  • Function : Author
K. Jackson
  • Function : Author
K. Youakim
  • Function : Author
C. Bradley
  • Function : Author

Abstract

The chemical abundances for five metal-poor stars in and towards the Galactic bulge have been determined from the H-band infrared spectroscopy taken with the RAVEN multi-object adaptive optics science demonstrator and the Infrared Camera and Spectrograph at the Subaru 8.2-m telescope. Three of these stars are in the Galactic bulge and have metallicities between -2.1 < [Fe/H] < -1.5, and high [α/Fe] ∼ +0.3, typical of Galactic disc and bulge stars in this metallicity range; [Al/Fe] and [N/Fe] are also high, whereas [C/Fe] < +0.3. An examination of their orbits suggests that two of these stars may be confined to the Galactic bulge and one is a halo trespasser, though proper motion values used to calculate orbits are quite uncertain. An additional two stars in the globular cluster M22 show [Fe/H] values consistent to within 1σ, although one of these two stars has [Fe/H] = -2.01 ± 0.09, which is on the low end for this cluster. The [α/Fe] and [Ni/Fe] values differ by 2σ, with the most metal-poor star showing significantly higher values for these elements. M22 is known to show element abundance variations, consistent with a multipopulation scenario though our results cannot discriminate this clearly given our abundance uncertainties. This is the first science demonstration of multi-object adaptive optics with high-resolution infrared spectroscopy, and we also discuss the feasibility of this technique for use in the upcoming era of 30-m class telescope facilities.
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Dates and versions

insu-03666206 , version 1 (12-05-2022)

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M. Lamb, K. Venn, D. Andersen, S. Oya, M. Shetrone, et al.. Using the multi-object adaptive optics demonstrator RAVEN to observe metal-poor stars in and towards the Galactic Centre. Monthly Notices of the Royal Astronomical Society, 2017, 465, pp.3536-3557. ⟨10.1093/mnras/stw2865⟩. ⟨insu-03666206⟩
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