Ages and kinematics of chemically selected, accreted Milky Way halo stars. Issue 4 (3rd February 2020)
- Record Type:
- Journal Article
- Title:
- Ages and kinematics of chemically selected, accreted Milky Way halo stars. Issue 4 (3rd February 2020)
- Main Title:
- Ages and kinematics of chemically selected, accreted Milky Way halo stars
- Authors:
- Das, Payel
Hawkins, Keith
Jofré, Paula - Abstract:
- ABSTRACT: We exploit the [Mg/Mn]-[Al/Fe] chemical abundance plane to help identify nearby halo stars in the 14 th data release from the APOGEE survey that have been accreted on to the Milky Way. Applying a Gaussian Mixture Model, we find a 'blob' of 856 likely accreted stars, with a low disc contamination rate of ∼7 per cent. Cross-matching the sample with the second data release from Gaia gives us access to parallaxes and apparent magnitudes, which place constraints on distances and intrinsic luminosities. Using a Bayesian isochrone pipeline, this enables us to estimate new ages for the accreted stars, with typical uncertainties of ∼20 per cent. This does not account for systematic uncertainties. Our new catalogue is further supplemented with estimates of orbital parameters. The blob stars span [Fe/H] between −2.5 to −0.5, and [Mg/Fe] between −0.1 to 0.5. They constitute ∼30 per cent of the metal-poor ([Fe/H] < −0.8) halo at [Fe/H] ∼ −1.4. Our new ages mainly range between 8 to 13 Gyr, with the oldest stars the metal-poorest, and with the highest [Mg/Fe] abundance. If the blob stars are assumed to belong to a single progenitor, the ages imply that star formation lasted 5 Gyr after which the system merged with our Milky Way around 8 Gyr ago. Dynamical arguments suggest that such a single progenitor would have had a total mass of $\sim 10^{11}\, \mathrm{M}_{\odot }$, similar to that found by other authors using chemical evolution models and simulations.
- Is Part Of:
- Monthly notices of the Royal Astronomical Society. Volume 493:Issue 4(2020)
- Journal:
- Monthly notices of the Royal Astronomical Society
- Issue:
- Volume 493:Issue 4(2020)
- Issue Display:
- Volume 493, Issue 4 (2020)
- Year:
- 2020
- Volume:
- 493
- Issue:
- 4
- Issue Sort Value:
- 2020-0493-0004-0000
- Page Start:
- 5195
- Page End:
- 5207
- Publication Date:
- 2020-02-03
- Subjects:
- Galaxy: abundances -- Galaxy: evolution -- Galaxy: halo -- Galaxy: kinematics and dynamics
Astronomy -- Periodicals
Periodicals
520.5 - Journal URLs:
- http://mnras.oxfordjournals.org/ ↗
http://onlinelibrary.wiley.com/journal/10.1111/(ISSN)1365-2966 ↗
http://www.blackwell-synergy.com/issuelist.asp?journal=mnr ↗
http://www.blackwell-synergy.com/loi/mnr ↗
http://ukcatalogue.oup.com/ ↗ - DOI:
- 10.1093/mnras/stz3537 ↗
- Languages:
- English
- ISSNs:
- 0035-8711
- Deposit Type:
- Legaldeposit
- View Content:
- Available online (eLD content is only available in our Reading Rooms) ↗
- Physical Locations:
- British Library DSC - 5943.000000
British Library DSC - BLDSS-3PM
British Library HMNTS - ELD Digital store - Ingest File:
- 15149.xml