The satellite galaxy plane of NGC 4490 in light of ΛCDM - Sparsity of similarly extreme analogs and a possible role of satellite pairs
arXiv:2405.06016 · doi:10.1051/0004-6361/202449954
Abstract
The galaxy system around NGC4490 was recently highlighted to display a flattened, kinematically correlated structure reminiscent of satellite galaxy planes around other hosts. Since known satellite planes are in tension with CDM expectations from cosmological simulations, we quantitatively assess for the first time the tension posed by the NGC4490 system. We measure the on-sky flattening as the major-to-minor axis ratio b/a of the satellite distribution and their line-of-sight kinematic correlation. Analogs are selected in the IllustrisTNG-50 simulation and their flattening and correlation are similarly measured. We confirm the strong kinematic coherence of all 12 observed objects with available line-of-sight velocities (of 14 in total): the northern ones approach and the southern ones recede relative to the host. The spatial distribution of all 14 objects is substantially flattened with b/a=0.38 (0.26 considering only the 12 objects with velocities). Such extreme arrangements are rare in the simulation at 0.21-0.35%. This would drop further if at least one of the two satellite objects without velocities is confirmed to follow the kinematic trend, and would become zero if both are rejected as non-members. We also identify a likely galaxy pair in the observed system, and find a similar pair in the best-matching simulated analog. Our findings establish NGC4490 as another strong example of a satellite plane in the Local Volume. This emphasizes that planes of satellites are a more general issue faced by CDM also beyond the Local Group. The tension with typical systems in simulations suggests that the observed one requires a specific formation scenario, potentially connected to the larger-scale galaxy alignment in its vicinity. The presence of galaxy pairs in the observed and a simulated system hints at the importance such groupings may have to understand satellite planes.
arXiv comment9 pages, 6 figures, 1 satellite galaxy plane. Accepted for publication in A&A. Abstract slightly abridged
References in corpus (50)
- Planck 2015 results. XIII. Cosmological parameters
- First results from the IllustrisTNG simulations: matter and galaxy clustering
- First results from the IllustrisTNG simulations: the stellar mass content of groups and clusters of galaxies
- First Results from the TNG50 Simulation: Galactic outflows driven by supernovae and black hole feedback
- Updated Nearby Galaxy Catalog
- A Vast Thin Plane of Co-rotating Dwarf Galaxies Orbiting the Andromeda Galaxy
- The great disk of Milky-Way satellites and cosmological sub-structures
- The VPOS: a vast polar structure of satellite galaxies, globular clusters and streams around the Milky Way
- The dark matter crisis: falsification of the current standard model of cosmology
- A whirling plane of satellite galaxies around Centaurus A challenges cold dark matter cosmology
- Confirmation of Faint Dwarf Galaxies in the M81 Group
- Co-orbiting satellite galaxy structures are still in conflict with the distribution of primordial dwarf galaxies
- Two Planes of Satellites in the Centaurus A Group
- The Planes of Satellite Galaxies Problem, Suggested Solutions, and Open Questions
- The preferred direction of infalling satellite galaxies in the Local Group
- The vast thin plane of M31 co-rotating dwarfs: an additional fossil signature of the M31 merger and of its considerable impact in the whole Local Group
- Action Dynamics of the Local Supercluster
- The Milky Way's Disk of Classical Satellite Galaxies in Light of Gaia DR2
- Velocity anti-correlation of diametrically opposed galaxy satellites in the low redshift universe
- A thousand shadows of Andromeda: rotating planes of satellites in the Millennium-II cosmological simulation
- Local Group Dwarf Elliptical Galaxies: II. Stellar Kinematics to Large Radii in NGC 147 and NGC 185
- Planes of satellite galaxies: when exceptions are the rule
- Did the Milky Way dwarf satellites enter the halo as a group?
- Making Counter-Orbiting Tidal Debris: The Origin of the Milky Way Disc of Satellites
- The M101 group complex: new dwarf galaxy candidates and spatial structure
- Planes of satellites around Milky Way/M31-mass galaxies in the FIRE simulations and comparisons with the Local Group
- MOND simulation suggests the origin of some peculiarities in the Local Group
- The multiplicity and anisotropy of galactic satellite accretion
- The coherent motion of Cen A dwarf satellite galaxies remains a challenge for CDM cosmology
- HST Proper Motions of NGC 147 and NGC 185: Orbital Histories and Test of Dynamically Coherent Andromeda Satellite Plane
- Tracing satellite planes in the Sculptor group: I. Discovery of three faint dwarf galaxies around NGC 253
- Modeling the Baryon Cycle in Low Mass Galaxy Encounters: the Case of NGC 4490 & NGC 4485
- Evidence for Early Filamentary Accretion from the Andromeda Galaxy's Thin Plane of Satellites
- The Clustering of Orbital Poles Induced by the LMC: Hints for the Origin of Planes of Satellites
- A Recent Major Merger Tale for the Closest Giant Elliptical Galaxy Centaurus A
- The alignment of SDSS satellites with the VPOS: effects of the survey footprint shape
- A Formation Scenario for the Disk of Satellites: Accretion of Satellites during Mergers
- Flattened structures of dwarf satellites around massive host galaxies in the MATLAS low-to-moderate density fields
- On the Co-Orbitation of Satellite Galaxies Along the Great Plane of Andromeda: NGC 147, NGC 185, and Expectations from Cosmological Simulations
- The orientation of planes of dwarf galaxies in the quasi-linear Universe
- Do halos that form early, have high concentration, are part of a pair, or contain a central galaxy potential host more pronounced planes of satellite galaxies?
- A co-rotating gas and satellite structure around the interacting galaxy pair NGC 4490/85
- A portrait of the Vast Polar Structure as a young phenomenon: hints from its member satellites
- On the Effect of the Large Magellanic Cloud on the Orbital Poles of Milky Way Satellite Galaxies
- Spatial and orbital planes of the Milky Way satellites: unusual but consistent with CDM
- FAST discovery of long tidal tails in NGC 4490/85
- A too-many dwarf satellite galaxies problem in the MATLAS low-to-moderate density fields
- The imprint of galaxy mergers on satellite planes in a cosmological context
- Satellite group infall into the Milky Way: exploring the Crater-Leo case with new HST proper motions
- Classifying the satellite plane membership of Centaurus A's dwarf galaxies using orbital alignment constraints
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- The Magellanic Clouds are very rare in the IllustrisTNG simulations
- Dwarf Galaxies in the MATLAS Survey: The satellite system of NGC474 under scrutiny with MUSE
- Andromeda's asymmetric satellite system as a challenge to cold dark matter cosmology
- 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
- The Delegate Survey: KOALA/AAOmega-IFU spectroscopy of three nearby dwarf galaxies