SIMBAD references

2020MNRAS.492.2161Z - Mon. Not. R. Astron. Soc., 492, 2161-2176 (2020/February-3)

Local RR Lyrae stars: native and alien.

ZINN R., CHEN X., LAYDEN A.C. and CASETTI-DINESCU D.I.

Abstract (from CDS):

Measurements of [Fe/H] and radial velocity are presented for 89 RR Lyrae (RRL) candidates within 6 kpc of the Sun. After the removal of two suspected non-RRLs, these stars were added to an existing data base, which yielded 464 RRLs with [Fe/H] on a homogeneous scale. Using data from the Gaia satellite (Data Release 2), we calculated the positions and space velocities for this sample. These data confirm the existence of a thin disc of RRL with [α/Fe] ∼ solar. The majority of the halo RRLs with large total energies have near-zero angular momenta about the Z-axis. Kinematically, these stars closely resemble the Gaia-Sausage/Gaia-Enceladus stars that others have proposed are debris from the merger of a large galaxy with the Milky Way. The metallicity and period distributions of the RRLs and their positions in the period-amplitude diagram suggest that this disrupted galaxy was as massive as the Large Magellanic Cloud and possibly greater.

Abstract Copyright: © 2019 The Author(s) Published by Oxford University Press on behalf of the Royal Astronomical Society

Journal keyword(s): stars: variables: RR Lyrae - Galaxy: formation - Galaxy: kinematics and dynamics

Status at CDS : Large table(s) will be appraised for possible ingestion in VizieR.

Simbad objects: 76

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2021.04.12-06:18:41

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