Authors: Arentsen, A; Starkenburg, E; Martin, Nicolas F.; Hill, V.; Ibata, R.; Kunder, A; Schultheis, M.; Venn, K; Zucker, D; Aguado, D; Carlberg, R; González hernández, J; Lardo, C; Longeard, N; Malhan, K; Navarro, J; Sánchez-Janssen, R; Sestito, F; Thomas, G; Youakim, K; Lewis, G; Simpson, J; Wan, Z
Venue: Monthly Notices of the Royal Astronomical Society: Letters
Type: Publication
Abstract: ABSTRACT Our Galaxy is known to contain a central boxy/peanut-shaped bulge, yet the importance of a classical, pressure-supported component within the central part of the Milky Way is still being debated. It should be most visible at low metallicity, a regime that has not yet been studied in detail. Using metallicity-sensitive narrow-band photometry, the Pristine Inner Galaxy Survey (PIGS) has collected a large sample of metal-poor ($\rm {[Fe/H]}\, \lt -1.0$) stars in the inner Galaxy to address this open question. We use PIGS to trace the meta...
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Impact:
4.9956686E-8
3.4179375E-9
73
28
/ Attention:
0
49
Topics: 
Stellar, planetary, and galactic studies
Astrophysics and Star Formation Studies
Astronomy and Astrophysical Research
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