The ISLAnds Project III: Variable Stars in Six Andromeda Dwarf Spheroidal Galaxies
arXiv:1710.09038 · doi:10.3847/1538-4357/aa9381
Abstract
We present a census of variable stars in six M31 dwarf spheroidal satellites observed with the Hubble Space Telescope. We detect 870 RR Lyrae (RRL) stars in the fields of And I (296), II (251), III (111), XV (117), XVI (8), XXVIII (87). We also detect a total of 15 Anomalous Cepheids, three Eclipsing Binaries, and seven field RRL stars compatible with being members of the M31 halo or the Giant Stellar Stream. We derive robust and homogeneous distances to the six galaxies using different methods based on the properties of the RRL stars. Working with the up-to-date set of Period-Wesenheit (, - ) relations published by Marconi et al., we obtain distance moduli of = [24.49, 24.16, 24.36, 24.42, 23.70, 24.43] mag (respectively), with systematic uncertainties of 0.08 mag and statistical uncertainties 0.11 mag. We have considered an enlarged sample of sixteen M31 satellites with published variability studies, and compared their pulsational observables (e.g., periods, amplitudes), with those of fifteen Milky Way satellites for which similar data are available. The properties of the (strictly old) RRL in both satellite systems do not show any significant difference. In particular, we found a strikingly similar correlation between the mean period distribution of the fundamental RRL pulsators (RRab) and the mean metallicities of the galaxies. This indicates that the old RRL progenitors were similar at the early stage in the two environments, suggesting very similar characteristics for the earliest stages of evolution of both satellite systems.
37 pages, 15 figures (some degraded), 29 tables, in emulateapj format. Accepted for publication in ApJ
References in corpus (21)
- Updated Electron-Conduction Opacities: The Impact on Low-Mass Stellar Models
- The Haunted Halos of Andromeda and Triangulum: A panorama of galaxy formation in action
- The PAndAS view of the Andromeda satellite system - II. Detailed properties of 23 M31 dwarf spheroidal galaxies
- Optical and Near-Infrared UBVRIJHK Photometry for the RR Lyrae stars in the Nearby Globular Cluster M4 (NGC 6121)
- On the distance of the globular cluster M4 (NGC 6121) using RR Lyrae stars: I. optical and near-infrared Period-Luminosity and Period-Wesenheit relations
- Weak Galactic halo--dwarf spheroidal connection from RR Lyrae stars
- Gaia Data Release 1 - The Cepheid & RR Lyrae star pipeline and its application to the south ecliptic pole region
- The Variable Stars of the Draco Dwarf Spheroidal Galaxy - Revisited
- Variable Stars in the Newly Discovered Milky Way Dwarf Spheroidal Satellite Canes Venatici I
- Infrared Tip of the Red Giant Branch and Distances to the Maffei/IC 342 Group
- Variable stars in Local Group Galaxies - II. Sculptor dSph
- On the RR Lyrae stars in globulars: IV. Centauri Optical UBVRI Photometry
- Comparing the observable properties of dwarf galaxies on and off the Andromeda plane
- The ACS LCID Project: RR Lyrae stars as tracers of old population gradients in the isolated dwarf spheroidal galaxy Tucana
- Comparing M31 and Milky Way Satellites: The Extended Star Formation Histories of Andromeda II and Andromeda XVI
- Weak Galactic Halo--Fornax dSph Connection from RR Lyrae Stars
- Synthetic properties of bright metal-poor variables. I. "Anomalous" Cepheids
- Variable stars and stellar populations in Andromeda XXV: III. A central cluster or the galaxy nucleus?
- DDO216-A1: a central globular cluster in a low-luminosity transition type galaxy
- The RR Lyrae Variable Population in the Phoenix Dwarf Galaxy
- A Photometric Study of the Outer Halo Globular Cluster NGC 5824
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- The Hubble Space Telescope Survey of M31 Satellite Galaxies I. RR Lyrae-based Distances and Refined 3D Geometric Structure
- TESS observations of Cepheid stars: first light results
- Solo dwarfs III: Exploring the orbital origins of isolated Local Group galaxies with Gaia Data Release 2
- Timing the r-Process Enrichment of the Ultra-Faint Dwarf Galaxy Reticulum II
- Identification of RR Lyrae stars in multiband, sparsely-sampled data from the Dark Energy Survey using template fitting and Random Forest classification
- The Isaac Newton Telescope monitoring survey of Local Group dwarf galaxies. I. Survey overview and first results for Andromeda I
- Variable stars in Local Group Galaxies -- V. The fast and early evolution of the low-mass Eridanus II dSph galaxy
- Metallicity of Galactic RR Lyrae from Optical and Infrared Light Curves: II. Period-Fourier-Metallicity Relations for First Overtone RR Lyrae
- A segmented period-luminosity relation for nearby extragalactic Scuti stars
- VVV catalog of ab-type RR Lyrae in the inner Galactic bulge
- RR Lyrae stars as probes of the outer Galactic halo: Chemical and kinematic analysis of a pilot sample