A Low-Mass Stellar-Debris Stream Associated with a Globular Cluster Pair in the Halo
arXiv:2007.05132 · doi:10.3847/2041-8213/aba49f
Abstract
There are expected to be physical relationships between the globular clusters (GCs) and stellar substructures in the Milky Way, not all of which have yet been found. We search for such substructures from a combined halo sample of SDSS blue horizontal-branch and SDSS+LAMOST RR Lyrae stars, cross-matched with astrometric information from DR2. This is a sample of old stars which are also excellent tracers of structures, ideal for searching for ancient relics in the outer stellar halo. By applying the neural-network-based method StarGO to the full 4D dynamical space of our sample, we rediscover the Sagittarius Stream, and find the debris of the -Enceladus-Sausage (GES) and the Sequoia events in the outer halo, as well as their linkages with several GCs. Most importantly, we find a new, low-mass, debris stream associated with a pair of GCs (NGC 5024 and NGC 5053), which we dub LMS-1. This stream has a very polar orbit, and occupies a region between 10 to 20 kpc from the Galactic center. NGC 5024 (M53), the more-massive of the associated GC pair, is very likely the nuclear star cluster of a now-disrupted dwarf galaxy progenitor, based on the results from N-body simulations.
arXiv comment10 pages, 4 figures, accepted for ApJL
References in corpus (46)
- Gaia Data Release 2. Summary of the contents and survey properties
- Gaia Data Release 2: The astrometric solution
- The merger that led to the formation of the Milky Way's inner stellar halo and thick disk
- SEGUE: A Spectroscopic Survey of 240,000 stars with g=14-20
- The mass distribution and gravitational potential of the Milky Way
- Co-formation of the Galactic disc and the stellar halo
- The Milky Way's Circular Velocity Curve to 60 kpc and an Estimate of the Dark Matter Halo Mass from Kinematics of ~2400 SDSS Blue Horizontal Branch Stars
- AGAMA: Action-based galaxy modelling architecture
- LAMOST Experiment for Galactic Understanding and Exploration (LEGUE) The survey science plan
- The SEGUE Stellar Parameter Pipeline. I. Description and Initial Validation Tests
- Evidence for Two Early Accretion Events That Built the Milky Way Stellar Halo
- Origin of the system of globular clusters in the Milky Way
- In disguise or out of reach: first clues about in-situ and accreted stars in the stellar halo of the Milky Way from Gaia DR2
- The VPOS: a vast polar structure of satellite galaxies, globular clusters and streams around the Milky Way
- Detection of a 63 Degree Cold Stellar Stream in the Sloan Digital Sky Survey
- The SEGUE Stellar Parameter Pipeline. II. Validation with Galactic Globular and Open Clusters
- Proper motions and dynamics of the Milky Way globular cluster system from Gaia DR2
- Assessing the Milky Way Satellites Associated with the Sagittarius Dwarf Spheroidal Galaxy
- Multiple retrograde substructures in the Galactic halo: A shattered view of Galactic history
- Mapping the substructure in the Galactic halo with the next generation of astrometric satellites
- N-body modeling of globular clusters: Masses, mass-to-light ratios and intermediate-mass black holes
- Ghostly Tributaries to the Milky Way: Charting the Halo's Stellar Streams with the Gaia DR2 catalogue
- The Hercules-Aquila Cloud
- Evidence for an accretion origin for the outer halo globular cluster system of M31
- Globular Cluster Systems in Nearby Dwarf Galaxies: III. Formation Efficiencies of Old Globular Clusters
- Dynamical Relics of the Ancient Galactic Halo
- Off the beaten path: Gaia reveals GD-1 stars outside of the main stream
- The Milky Way Halo in Action Space
- Origin of the excess of high-energy retrograde stars in the Galactic halo
- The SEGUE K giant survey II: A Catalog of Distance Determinations for the SEGUE K giants in the Galactic Halo
- Absolute HST Proper Motion (HSTPROMO) of Distant Milky Way Globular Clusters: Galactocentric Space Velocities and the Milky Way Mass
- Exploring the Properties of the M31 Halo Globular Cluster System
- Common origin for Hercules-Aquila and Virgo Clouds in Gaia DR2
- StarGO: A New Method to Identify the Galactic Origins of Halo Stars
- An all-sky proper motion map of the Sagittarius stream using Gaia DR2
- A panoramic landscape of the Sagittarius stream in Gaia DR2 revealed with the STREAMFINDER spyglass
- Full 5D characterisation of the Sagittarius stream with Gaia DR2 RR Lyrae
- The outer halo globular cluster system of M31 - III. Relationship to the stellar halo
- A wide-field photometric survey for extratidal tails around five metal-poor globular clusters in the Galactic halo
- Strong RR Lyrae excess in the Hercules-Aquila Cloud
- Probing the galactic halo with RR Lyrae stars I: The catalog
- The Milky Way's stellar streams and globular clusters do not align in a Vast Polar Structure
- Revealing the Complicated Story of the Cetus Stream with StarGO
- Phase-space correlation in stellar streams of the Milky Way halo: The clash of Kshir and GD-1
- Chemical Abundances in NGC 5053: A Very Metal-Poor and Dynamically Complex Globular Cluster
- A Search for Extra-Tidal RR Lyrae in the Globular Cluster NGC 5024 and NGC 5053
Cited by in corpus (63)
- Evidence from the H3 Survey that the Stellar Halo is Entirely Comprised of Substructure
- The Global Dynamical Atlas of the Milky Way mergers: Constraints from Gaia EDR3 based orbits of globular clusters, stellar streams and satellite galaxies
- The chemical characterisation of halo substructure in the Milky Way based on APOGEE
- The Poor Old Heart of the Milky Way
- The Chemo-Dynamical Groups of Galactic Globular Clusters
- galstreams: A Library of Milky Way Stellar Stream Footprints and Tracks
- : The Orbital and Chemical Properties of One Dozen Stellar Streams
- The GALAH Survey: Chemical tagging and chrono-chemodynamics of accreted halo stars with GALAH+ DR3 and eDR3
- GASTRO library I: the simulated chemodynamical properties of several GSE-like stellar halos
- Dynamically Tagged Groups of Very Metal-poor Halo Stars from the HK and Hamburg/ESO Surveys
- 3D Morphology of Open Clusters in the Solar Neighborhood with Gaia EDR3 II: Hierarchical Star Formation Revealed by Spatial and Kinematic Substructures
- The Kinematic Properties of Milky Way Stellar Halo Populations
- Stellar Escape from Globular Clusters. I. Escape Mechanisms and Properties at Ejection
- Substructure in the stellar halo near the Sun. II. Characterisation of independent structures
- Substructure in the stellar halo near the Sun. I. Data-driven clustering in Integrals of Motion space
- The distribution of globular clusters in kinematic spaces does not trace the accretion history of the host galaxy
- The Pristine survey -- XVI. The metallicity of 26 stellar streams around the Milky Way detected with the STREAMFINDER in Gaia EDR3
- The Complexity of the Cetus Stream Unveiled from the Fusion of STREAMFINDER and StarGO
- Dynamically Tagged Groups of Metal-Poor Stars from the Best \& Brightest Survey
- Probing the Galactic Halo with RR Lyrae Stars. II. The Substructures of the Milky Way
- Disruption of Hierarchical Clustering in the Vela OB2 Complex and the Cluster Pair Collinder 135 and UBC7 with Gaia EDR3: Evidence of Supernova Quenching
- Chemo-Dynamically Tagged Groups of CEMP Stars in the Halo of the Milky Way. I. Untangling the Origins of CEMP- and CEMP-no Stars
- The R-Process Alliance: Chemo-Dynamically Tagged Groups II. An Extended Sample of Halo -Process-Enhanced Stars
- APOGEE spectroscopic evidence for chemical anomalies in dwarf galaxies: The case of M~54 and Sagittarius
- Dynamically Tagged Groups of Metal-Poor Stars II. The Radial Velocity Experiment Data Release 6
- The observable properties of galaxy accretion events in Milky Way-like galaxies in the FIRE-2 cosmological simulations
- The Unmixed Debris of Gaia-Sausage/Enceladus in the Form of a Pair of Halo Stellar Overdensities
- Phase-space Properties and Chemistry of the Sagittarius Stellar Stream Down to the Extremely Metal-poor () Regime
- Contribution of Gaia Sausage to the Galactic Stellar Halo Revealed by K Giants and Blue Horizontal Branch Stars from the Large Sky Area Multi-Object Fiber Spectroscopic Telescope, Sloan Digital Sky Survey, and Gaia
- Exploring the diversity and similarity of radially anisotropic Milky Way-like stellar haloes: implications for disrupted dwarf galaxy searches
- The Pristine survey -- XV. A CFHT ESPaDOnS view on the Milky Way halo and disc populations
- A Blueprint for the Milky Way's Stellar Populations. III. Spatial Distributions and Population Fractions of Local Halo Stars
- Extending the Chemical Reach of the H3 Survey: Detailed Abundances of the Dwarf-galaxy Stellar Stream Wukong/LMS-1
- Four-hundred Very Metal-poor Stars Studied with LAMOST and Subaru. III. Dynamically Tagged Groups and Chemodynamical Properties
- Dynamics of Stellar Disk Tilting from Satellite Mergers
- Charting Galactic Accelerations with Stellar Streams and Machine Learning
- Exploring the chemodynamics of metal-poor stellar populations
- The SDSS-Gaia View of the Color-Magnitude Relation for Blue Horizontal-branch Stars
- Potential Black Hole Seeding of the Spiral Galaxy NGC 4424 via an Infalling Star Cluster
- Extra-tidal star candidates in globular clusters of the Sagittarius dwarf spheroidal galaxy
- Hidden deep in the halo: selection of a reduced proper motion halo catalogue and mining retrograde streams in the velocity space
- The S-PLUS Ultra-Short Survey: first data release
- L-GALAXIES 2020: The formation and chemical evolution of stellar haloes in Milky Way Analogues and galaxy clusters
- Globular Cluster Intrinsic Iron Abundance Spreads: II. Protocluster Metallicities and the Age-Metallicity Relations of Milky Way Progenitors
- RR Lyrae stars as probes of the outer Galactic halo: Chemical and kinematic analysis of a pilot sample
- A Ghost in Boötes: The Least Luminous Disrupted Dwarf Galaxy
- Dynamical Origin for the Collinder 132-Gulliver 21 Stream: A Mixture of three Co-Moving Populations with an Age Difference of 250 Myr
- HALO7D III: Chemical Abundances of Milky Way Halo Stars from Medium Resolution Spectra
- Dynamical mirages: how bar-induced resonant trapping can mimic substructure clustering in dynamical parameter spaces
- Detection of the actinide Th in an r-process-enhanced star with accretion origin
- Revealing the Milky Way's Most Recent Major Merger with a Gaia EDR3 Catalog of Machine-Learned Line-of-Sight Velocities
- Discovery of the shell structure via break radii in the outer halo of the Milky Way
- A Dwarf Galaxy Debris Stream Associated with Palomar 1 and the Anticenter Stream
- Globular clusters in \textsc{OrbIT}: complete dynamical characterisation of the globular cluster population of the Milky Way through updated orbital reconstruction
- The Origin of Young Stellar Populations in NGC 1783: Accretion of External Stars
- Main-sequence Turnoff Stars as Probes of the Ancient Galactic Relic: Chemo-dynamical Analysis of a Pilot Sample
- The Pristine survey. XXVI. Chemical abundances of subgiant stars of the extremelymetal-poor stream C-19
- Identifying substructure associations in the Milky Way halo using chemo-kinematic tagging
- Light Element Abundances and Multiple Populations in M53
- Unveiling Galactic substructures with M Giant stars: A kinematic and chemical study based on LAMOST DR9, Gaia DR3 and APOGEE DR17
- HR-GO II: chemical abundances of low- retrograde dynamically-tagged-groups: Revealing Thamnos as a very metal-poor substructure
- Identification of a dwarf galaxy stream in Gaia, and its possible association with the VPOS structure
- HE0144-4657: A Carbon-Enhanced Ultra Metal-Poor Star ([Fe/H] ~ -4.1) from the Helmi Stream Disrupted Dwarf Galaxy