Satellite group infall into the Milky Way: exploring the Crater-Leo case with new HST proper motions
arXiv:2404.16110 · doi:10.1051/0004-6361/202449985
Abstract
Context. Within Cold Dark Matter (CDM) simulations, Milky Way-like galaxies accrete some of their satellite galaxies in groups of 3-5 members rather than individually. It was also suggested that this might be the reason behind the origin of satellite planes. Objects accreted in groups are expected to share similar specific total energy and angular momentum, and also identical orbital planes and directions. Aims. Looking at observations of Milky Way satellites, the dwarf galaxies Leo II, IV, V, Crater II, and the star cluster Crater 1 were proposed to be a vestige of group infall. The suggested "Crater-Leo group" shows a coherent distance gradient and all these objects align along a great circle on the sky. We use proper motion data to investigate whether the phase-space distribution of the members of the proposed group are indeed consistent with group infall. Methods. To further investigate this possibility, we use Gaia Data Release 3 (DR3) and new Hubble Space Telescope (HST) proper motions, mas yr for Leo IV and mas yr for Leo V, to derive accurate orbital properties for the proposed group objects. In addition, we explore other possible members of this putative association. Results. Leo II, Leo IV, and Crater 1 show orbital properties consistent with those we predict from assuming group infall. However, our results suggest that Crater II was not accreted with the rest of the objects. If confirmed with increasingly accurate proper motions in the future, the Crater-Leo objects appear to constitute the first identified case of a cosmologically expected, typical group infall event, as opposed to the highly hierarchical Magellanic Cloud system.
arXiv commentAccepted for publication in A&A on 23-04-2024. 20 pages, 18 figures, 5 tables
References in corpus (80)
- SciPy 1.0--Fundamental Algorithms for Scientific Computing in Python
- Array Programming with NumPy
- emcee: The MCMC Hammer
- Binary companions of evolved stars in APOGEE DR14: Search method and catalog of ~5,000 companions
- Local Kinematics and the Local Standard of Rest
- The Aquarius Project: the subhalos of galactic halos
- The observed properties of dwarf galaxies in and around the Local Group
- galpy: A Python Library for Galactic Dynamics
- A geometric distance measurement to the Galactic Center black hole with 0.3% uncertainty
- Cats and Dogs, Hair and A Hero: A Quintet of New Milky Way Companions
- The Universal Stellar Mass-Stellar Metallicity Relation for Dwarf Galaxies
- The subhalo populations of LCDM dark haloes
- Beasts of the Southern Wild: Discovery of nine Ultra Faint satellites in the vicinity of the Magellanic Clouds
- Eight Ultra-faint Galaxy Candidates Discovered in Year Two of the Dark Energy Survey
- A Vast Thin Plane of Co-rotating Dwarf Galaxies Orbiting the Andromeda Galaxy
- The Star Formation Histories of Local Group Dwarf Galaxies I. Hubble Space Telescope / Wide Field Planetary Camera 2 Observations
- Mean proper motions, space orbits and velocity dispersion profiles of Galactic globular clusters derived from Gaia DR2 data
- The VPOS: a vast polar structure of satellite galaxies, globular clusters and streams around the Milky Way
- A Curious New Milky Way Satellite in Ursa Major
- The Quenching of the Ultra-Faint Dwarf Galaxies in the Reionization Era
- Tango for three: Sagittarius, LMC, and the Milky Way
- Gaia DR2 Proper Motions of Dwarf Galaxies within 420 kpc: Orbits, Milky Way Mass, Tidal Influences, Planar Alignments, and Group Infall
- The feeble giant. Discovery of a large and diffuse Milky Way dwarf galaxy in the constellation of Crater
- Comparing the properties of local globular cluster systems: implications for the formation of the Galactic halo
- Hunting for the Dark Matter Wake Induced by the Large Magellanic Cloud
- A MegaCam Survey of Outer Halo Satellites. III. Photometric and Structural Parameters
- A whirling plane of satellite galaxies around Centaurus A challenges cold dark matter cosmology
- Small Dwarf Galaxies Within Larger Dwarfs: Why Some Are Luminous While Most Go Dark
- The Orbital Histories of Magellanic Satellites Using Gaia DR2 Proper Motions
- And yet it moves: The dangers of artificially fixing the Milky Way center of mass in the presence of a massive Large Magellanic Cloud
- Leo V: A Companion of a Companion of the Milky Way Galaxy
- Associations of Dwarf Galaxies
- Sweating the small stuff: simulating dwarf galaxies, ultra-faint dwarf galaxies, and their own tiny satellites
- Infall of substructures onto a Milky Way-like dark halo
- Squelched Galaxies and Dark Halos
- Gaia early DR3 systemic motions of Local Group dwarf galaxies and orbital properties with a massive Large Magellanic Cloud
- Two Planes of Satellites in the Centaurus A Group
- The Missing Satellites of the Magellanic Clouds? Gaia Proper Motions of the Recently Discovered Ultra-Faint Galaxies
- Spectroscopic Confirmation of the Dwarf Galaxies Hydra II and Pisces II and the Globular Cluster Laevens 1
- The M31 Velocity Vector. I. Hubble Space Telescope Proper Motion Measurements
- Crater 2: An Extremely Cold Dark Matter Halo
- The Anisotropic Distribution of M 31 Satellite Galaxies: A Polar Great Plane of Early-Type Companions
- The satellite distribution of M31
- The Milky Way's Disk of Classical Satellite Galaxies in Light of Gaia DR2
- A Hero's Dark Horse: Discovery of an Ultra-Faint Milky Way Satellite in Pegasus
- Local Group Dwarf Elliptical Galaxies: II. Stellar Kinematics to Large Radii in NGC 147 and NGC 185
- ATLAS lifts the Cup: Discovery of a New Milky Way satellite in Crater
- Kinematics of Antlia 2 and Crater 2 from The Southern Stellar Stream Spectroscopic Survey (S5)
- Proper motions of Milky Way Ultra-Faint satellites with DR2 DES DR1
- The predicted luminous satellite populations around SMC and LMC-mass galaxies - A missing satellite problem around the LMC?
- Reflex motion in the Milky Way stellar halo resulting from the Large Magellanic Cloud infall
- Clues to the "Magellanic Galaxy" from Cosmological Simulations
- The Spatial Distribution of Galactic Satellites in the LCDM Cosmology
- The Leo IV dwarf spheroidal galaxy: color-magnitude diagram and pulsating stars
- The multiplicity and anisotropy of galactic satellite accretion
- HST Proper Motions of NGC 147 and NGC 185: Orbital Histories and Test of Dynamically Coherent Andromeda Satellite Plane
- A Hubble Space Telescope Study of the Enigmatic Milky Way Halo Globular Cluster Crater
- Dark and luminous satellites of LMC-mass galaxies in the FIRE simulations
- Testing the two planes of satellites in the Centaurus Group
- The binary fraction of stars in dwarf galaxies: the case of Leo II
- The enigmatic pair of dwarf galaxies Leo IV and Leo V: coincidence or common origin?
- VLT Spectroscopy of Ultra-Faint Dwarf Galaxies. 1. Boötes I, Leo IV, Leo V
- Dynamical Histories of the Crater II and Hercules Dwarf Galaxies
- The evolved stars of Leo II dSph galaxy from near-infrared UKIRT/WFCAM observations
- The velocity anisotropy of the Milky Way satellite system
- HST/ACS Direct Ages of the Dwarf Elliptical Galaxies NGC 147 and NGC 185
- The Binary Galaxies NGC 147 And NGC 185
- The Clustering of Orbital Poles Induced by the LMC: Hints for the Origin of Planes of Satellites
- Pre-processing, group accretion and the orbital trajectories of associated subhaloes
- Proper Motion of the Leo II Dwarf Galaxy Based On Hubble Space Telescope Imaging
- Dynamical model of the Milky Way using APOGEE and Gaia data
- A DECam View of the Diffuse Dwarf Galaxy Crater II: Variable Stars
- Galaxy Pairs in the Local Group
- Search for globular clusters associated with the Milky Way dwarf galaxies using Gaia DR2
- Globular Clusters in Dwarf Galaxies
- Signatures of Tidal Disruption in Ultra-Faint Dwarf Galaxies: A Combined HST, Gaia, and MMT/Hectochelle Study of Leo V
- On the Effect of the Large Magellanic Cloud on the Orbital Poles of Milky Way Satellite Galaxies
- Ultrafaint Dwarf Galaxy Candidates in the M81 Group: Signatures of Group Accretion
- A DECam View of the Diffuse Dwarf Galaxy Crater II: The Colour-Magnitude Diagram
- NGC 147, NGC 185 and CassII: a genetic approach to orbital properties, star formation and tidal debris
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- The satellite galaxy plane of NGC 4490 in light of ΛCDM - Sparsity of similarly extreme analogs and a possible role of satellite pairs
- Dwarf Galaxies in the MATLAS Survey: The satellite system of NGC474 under scrutiny with MUSE
- An LBT view of the co-rotating group of galaxies around NGC 2750: Deep imaging and new satellite candidates
- Testing a proposed "planarity" tool for studying satellite systems: On the alleged consistency of Milky Way satellite galaxy planes with CDM
- The long-term stability of the Vast Polar Structure and its connection to a possible previous passage of the LMC
- Investigating the origin of the Milky Way streams. A revised look at their orbital pole distribution in light of precession effects