The Pristine survey XIII: Uncovering the very metal-poor tail of the thin disc

  • Emma Fernández-Alvar
  • , Georges Kordopatis
  • , Vanessa Hill
  • , Else Starkenburg
  • , Akshara Viswanathan
  • , Nicolas F. Martin
  • , Guillaume F. Thomas
  • , Julio F. Navarro
  • , Khyati Malhan
  • , Federico Sestito
  • , Jonay I. González Hernández
  • , Raymond G. Carlberg

Research output: Contribution to journalArticlepeer-review

32 Citations (Scopus)
5 Downloads (Pure)

Abstract

We evaluate the rotational velocity of stars observed by the Pristine survey towards the Galactic anticentre, spanning a wide range of metallicities from the extremely metal-poor regime ($\mathrm{[Fe/H]} -1.5$. Furthermore, we detect signatures of a "heated disc", the so-called Splash, at metallicities higher than $\sim-1.5$. Finally, at $\mathrm{[Fe/H]} < -1.5$ our anticentre sample is dominated by a kinematical halo with a net prograde motion.
Original languageUndefined/Unknown
JournalMonthly Notices of the Royal Astronomical Society (MNRAS)
DOIs
Publication statusPublished - 7 Jun 2021

Keywords

  • astro-ph.GA
  • astro-ph.IM
  • astro-ph.SR

Cite this