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Characterization of high-velocity stars in the S-PLUS internal fourth data release.
- Source :
- Monthly Notices of the Royal Astronomical Society; Jan2024, Vol. 527 Issue 3, p6173-6188, 16p
- Publication Year :
- 2024
-
Abstract
- In general, the atypical high velocity of some stars in the Galaxy can only be explained by invoking acceleration mechanisms related to extreme astrophysical events in the Milky Way. Using astrometric data from Gaia and the photometric information in 12 filters of the S-PLUS, we performed a kinematic, dynamical, and chemical analysis of 64 stars with Galactocentric velocities higher than 400 |$\mathrm{km\, s}^{-1}$|. All the stars are gravitationally bound to the Galaxy and exhibit halo kinematics. Some of the stars could be remnants of structures such as the Sequoia and the Gaia-Sausage/Enceladus. Supported by orbital and chemical analysis, we identified Gaia DR3 5401875170994688896 as a star likely to be originated at the centre of the Galaxy. Application of a machine learning technique to the S-PLUS photometric data allows us to obtain very good estimates of magnesium abundances for this sample of high-velocity stars. [ABSTRACT FROM AUTHOR]
- Subjects :
- STARS
DATA release
MILKY Way
STELLAR dynamics
INFORMATION filtering
ASTROMETRY
Subjects
Details
- Language :
- English
- ISSN :
- 00358711
- Volume :
- 527
- Issue :
- 3
- Database :
- Complementary Index
- Journal :
- Monthly Notices of the Royal Astronomical Society
- Publication Type :
- Academic Journal
- Accession number :
- 175059557
- Full Text :
- https://doi.org/10.1093/mnras/stad3610