Stellar Stream and Halo Structure in the Andromeda Galaxy From a Subaru/Hyper Suprime-Cam Survey
arXiv:1712.03654 · doi:10.3847/1538-4357/aaa129
Abstract
We present wide and deep photometry of the northwest part of the halo of the Andromeda galaxy (M31) using Hyper Suprime-Cam on the Subaru Telescope. The survey covers 9.2 deg field in the , , and bands and shows a clear red giant branch (RGB) of M31's halo stars and a pronounced red clump (RC) feature. The spatial distribution of RC stars shows a prominent stream feature, the North Western (NW) Stream, and a diffuse substructure in the south part of our survey field. We estimate the distances based on the RC method and obtain = 24.63(random)(systematic) and 24.29(random)(systematic) mag for the NW stream and diffuse substructure, respectively, implying that the NW Stream is located behind M31, whereas the diffuse substructure is located in front. We also estimate line-of-sight distances along the NW Stream and find that the south part of the stream is 20 kpc closer to us relative to the north part. The distance to the NW Stream inferred from the isochrone fitting to the color-magnitude diagram favors the RC-based distance, but the TRGB-based distance estimated for -selected RGB stars does not agree with it. The surface number density distribution of RC stars across the NW Stream is found to be approximately Gaussian with a FWHM of 25 arcmin (5.7 kpc), with a slight skew to the south-west side. That along the NW Stream shows a complicated structure including variations in number density and a significant gap in the stream.
24 pages, 18 figures, accepted for publication in ApJ
References in corpus (23)
- The Kinematics of the Ultra-Faint Milky Way Satellites: Solving the Missing Satellite Problem
- Beasts of the Southern Wild: Discovery of nine Ultra Faint satellites in the vicinity of the Magellanic Clouds
- A Vast Thin Plane of Co-rotating Dwarf Galaxies Orbiting the Andromeda Galaxy
- The Hyper Suprime-Cam Software Pipeline
- The Observed properties of Dark Matter on small spatial scales
- Hundreds of Milky Way Satellites? Luminosity Bias in the Satellite Luminosity Function
- The Luminosity Function of the Milky Way Satellites
- The Metal-Poor Halo of the Andromeda Spiral Galaxy (M31)
- The Invisibles: A Detection Algorithm to Trace the Faintest Milky Way Satellites
- The number and size of subhalo-induced gaps in stellar streams
- Investigating the Andromeda Stream: III. A Young Shell System in M31
- The outer halo globular cluster system of M31 - I. The final PAndAS catalogue
- Global Properties of M31's Stellar Halo from the SPLASH Survey. I. Surface Brightness Profile
- A New Method for Isolating M31 Red Giant Stars: The Discovery of Stars out to a Radial Distance of 165 Kiloparsecs
- The outer halo globular cluster system of M31 - II. Kinematics
- The Tip of the Red Giant Branch Distances to Type Ia Supernova Host Galaxies. IV. Color Dependence and Zero-Point Calibration
- The PAndAS Field of Streams: stellar structures in the Milky Way halo toward Andromeda and Triangulum
- Global Properties of M31's Stellar Halo from the SPLASH Survey: II. Metallicity Profile
- Discovery of a Faint Old Stellar System at 150 kpc
- Formation of the Andromeda Giant Stream: Asymmetric Structure and Disc Progenitor
- Resolved stellar streams around NGC4631 from a Subaru/Hyper Suprime-Cam survey
- HST Imaging of the Local Volume Dwarf Galaxies Pisces A&B: Prototypes for Local Group Dwarfs
- The nature of the progenitor of the M31 North-western stream: globular clusters as milestones of its orbit
Cited by in corpus (19)
- The eROSITA Final Equatorial-Depth Survey (eFEDS): Catalog of galaxy clusters and groups
- Halo Concentration, Galaxy Red Fraction, and Gas Properties of Optically-defined Merging Clusters
- Euclid: Early Release Observations -- Deep anatomy of nearby galaxies
- Stellar halos from The Dragonfly Edge-on Galaxies Survey
- Stellar population and structural properties of dwarf galaxies and young stellar systems in the M81 group
- Spatially Resolved Metal Loss from M31
- Project AMIGA: Distance and Metallicity Gradients Along Andromeda's Giant Southern Stream from the Red Clump
- Active gas features in three HSC-SSP CAMIRA clusters revealed by high angular resolution analysis of MUSTANG-2 SZE and XXL X-ray observations
- A Tale of a Tail: A Tidally-Disrupting Ultra-Diffuse Galaxy in the M81 Group
- Statistical properties of substructures around Milky Way-sized haloes and their implications for the formation of stellar streams
- Subaru Hyper Suprime-Cam Survey of Cygnus OB2 Complex -- I: Introduction, Photometry and Source Catalog
- Metallicities of Outer Halo M31 Globular Clusters from Integrated Light Calcium-II Triplet Spectroscopy
- A Dwarf Disrupting -- Andromeda XXVII and the North West Stream
- Scaling relations of X-ray Luminous Clusters in the Hyper Suprime-Cam Subaru Strategic Program Field
- A New Polar Ring Galaxy Discovered in the COSMOS Field
- One Stream or Two -- Exploring Andromeda's North West Stream
- Analysing Ultra High Energy Cosmic Rays' Anisotropy in Gravity Theory
- HSC-XXL : Baryon budget of the 136 XXL Groups and Clusters
- Properties of the Lower Segment of M31's North West Stream