Reading the tea leaves in the - and - diagrams: dry and gaseous mergers with remnant angular momentum
arXiv:2210.09557 · doi:10.1093/mnras/stad087
Abstract
We recently revealed that bulges and elliptical galaxies broadly define distinct, super-linear relations in the - diagram, with the order-of-magnitude lower ratios in the elliptical galaxies due to major (disc-destroying, elliptical-building) dry mergers. Here we present a more nuanced picture. Galaxy mergers, in which the net orbital angular momentum does not cancel, can lead to systems with a rotating disc. This situation can occur with either wet (gas-rich) mergers involving one or two spiral galaxies, e.g., NGC~5128, or dry (relatively gas-poor) collisions involving one or two lenticular galaxies, e.g., NGC~5813. The spheroid and disc masses of the progenitor galaxies and merger remnant dictate the shift in the - and - diagrams. We show how this explains the (previously excluded merger remnant) Sersic S0 galaxies near the bottom of the elliptical sequence and core-Sersic S0 galaxies at the top of the bulge sequence, neither of which are faded spiral galaxies. Different evolutionary pathways in the scaling diagrams are discussed. We also introduce two ellicular (ES) galaxy types, explore the location of brightest cluster galaxies and stripped `compact elliptical' galaxies in the - diagram, and present a new merger-built - relation which may prove helpful for studies of nanohertz gravitational waves. This work effectively brings into the fold many systems previously considered outliers with either overly massive or undermassive black holes relative to the near-linear - `red sequence' patched together with select bulges and elliptical galaxies.
Revised version after minor comments from the referee and tweaks from the authors. (15 pages of main text and figures, plus 8 pages of Appendix and References.)
References in corpus (76)
- SciPy 1.0--Fundamental Algorithms for Scientific Computing in Python
- Array Programming with NumPy
- Cold streams in early massive hot haloes as the main mode of galaxy formation
- Simba: Cosmological Simulations with Black Hole Growth and Feedback
- The NANOGrav 12.5-year Data Set: Search For An Isotropic Stochastic Gravitational-Wave Background
- A distance to the Large Magellanic Cloud that is precise to one per cent
- Star formation efficiency in galaxy interactions and mergers: a statistical study
- Galaxy Merger Morphologies and Time-Scales from Simulations of Equal-Mass Gas-Rich Disc Mergers
- On the evidence for a common-spectrum process in the search for the nanohertz gravitational-wave background with the Parkes Pulsar Timing Array
- The dark nemesis of galaxy formation: why hot haloes trigger black hole growth and bring star formation to an end
- Common-red-signal analysis with 24-yr high-precision timing of the European Pulsar Timing Array: Inferences in the stochastic gravitational-wave background search
- Imfit: A Fast, Flexible New Program for Astronomical Image Fitting
- The influence of gas on the structure of merger remnants
- Black Holes on FIRE: Stellar Feedback Limits Early Feeding of Galactic Nuclei
- The black hole mass -- stellar velocity dispersion correlation: bulges versus pseudobulges
- The mass relations between supermassive black holes and their host galaxies at 1<z<2 with HST-WFC3
- From Supermassive Black Holes to Dwarf Elliptical Nuclei: a Mass Continuum
- Supermassive black holes in cosmological simulations I: M_BH-M_star relation and black hole mass function
- Evidence for Merger Remnants in Early-Type Host Galaxies of Low-Redshift QSOs
- Intracluster light and the extended stellar envelopes of cD galaxies: An analytical description
- The Black Hole Mass-Bulge Luminosity Relationship for Active Galactic Nuclei from Reverberation Mapping and Hubble Space Telescope Imaging
- Composite Bulges: The Coexistence of Classical Bulges and Disky Pseudobulges in S0 and Spiral Galaxies
- A Very Deep Chandra Observation of the Galaxy Group NGC 5813: AGN Shocks, Feedback, and Outburst History
- The (black hole)-bulge mass scaling relation at low masses
- Black Hole Mass Scaling Relations for Early-Type Galaxies: - and -
- Hidden AGN in dwarf galaxies revealed by MaNGA: light echoes, off-nuclear wanderers, and a new broad-line AGN
- Updated Mass Scaling Relations for Nuclear Star Clusters and a Comparison to Supermassive Black Holes
- The First Spectroscopically Resolved Sub-parsec Orbit of a Supermassive Binary Black Hole
- The Host Galaxy and Central Engine of the Dwarf AGN POX 52
- Improved Dynamical Constraints on the Mass of the central Black Hole in NGC 404
- Two new confirmed massive relic galaxies: red nuggets in the present-day Universe
- Hiding in plain sight: An abundance of compact massive spheroids in the local Universe
- The initial mass function of a massive relic galaxy
- On the interdependence of galaxy morphology, star formation, and environment in massive galaxies in the nearby Universe
- Revealing Hidden Substructures in the - Diagram, and Refining the Bend in the - Relation
- Preparing for low surface brightness science with the Vera C. Rubin Observatory: characterisation of tidal features from mock images
- Revealing the intermediate-mass black hole at the heart of the dwarf galaxy NGC 404 with sub-parsec resolution ALMA observations
- A local baseline of the black hole mass scaling relations for active galaxies. IV. Correlations between and host galaxy , stellar mass, and luminosity
- Black Hole Mass Measurements of Radio Galaxies NGC 315 and NGC 4261 Using ALMA CO Observations
- Stellar Photometric Structures of the Host Galaxies of Nearby Type 1 Active Galactic Nuclei
- Dynamical evolution of cosmic supermassive binary black holes and their gravitational wave radiation
- Correlation Between the Total Gravitating Mass of Groups and Clusters and the Supermassive Black Hole Mass of Brightest Galaxies
- A Morphological and Statistical Analysis of Ansae in Barred Galaxies
- The Brightest Cluster Galaxy in Abell 85: The Largest Core Known so far
- Measuring supermassive black holes with gas kinematics: the active S0 galaxy NGC 3998
- Appreciating mergers for understanding the non-linear - and - relations, updated herein, and the implications for the (reduced) role of AGN feedback
- Infrared Surface Brightness Fluctuation Distances for MASSIVE and Type Ia Supernova Host Galaxies
- A Recent Major Merger Tale for the Closest Giant Elliptical Galaxy Centaurus A
- A galaxy classification grid that better recognises early-type galaxy morphology
- Prevalence of Tidal Interactions among Local Seyfert Galaxies
- Stellar Mass-to-light Ratios: Composite Bulge+Disk Models and the Baryonic Tully-Fisher Relation
- Implications for the origin of dwarf early-type galaxies: a detailed look at the isolated rotating dwarf early-type galaxy CG 611, with ramifications for the Fundamental Plane's (S_K)^2 kinematic scaling and the spin-ellipticity diagram
- Consistency of the Parkes Pulsar Timing Array Signal with a Nanohertz Gravitational-wave Background
- Defining the (Black Hole)-Spheroid Connection with the Discovery of Morphology-Dependent Substructure in the -- and -- Diagrams: New Tests for Advanced Theories and Realistic Simulations
- . I. Understanding galaxy sizes, associated luminosity densities, and the artificial division of the early-type galaxy population
- Disky elliptical galaxies and the allegedly over-massive black hole in the compact massive `ES' galaxy NGC 1271
- Expected intermediate-mass black holes in the Virgo cluster. I. Early-type galaxies
- WISDOM Project -- VII. Molecular gas measurement of the supermassive black hole mass in NGC 7052
- A search for active galactic nuclei in low-mass compact galaxies
- NGC5252: a pair of radio-emitting active galactic nuclei?
- The quest for the largest depleted galaxy core: supermassive black hole binaries and stalled in-falling satellites
- A consistency-test for determining whether ultra-compact dwarf galaxies could be the remnant nuclei of threshed galaxies
- Disc cloaking: Establishing a lower limit to the number density of local compact massive spheroids/bulges and the potential fate of some high-z red nuggets
- Large-scale structure and galaxy motions in the Leo/Cancer constellations
- Building the peanut: simulations and observations of peanut-shaped structures and ansae in face-on disk galaxies
- The (Black Hole Mass)-(Spheroid Stellar Density) Relations: -- (and --) and --
- The SLUGGS Survey: Trails of SLUGGS galaxies in a modified spin-ellipticity diagram
- GALFIT-CORSAIR: implementing the core-Sersic model into GALFIT
- Potential Black Hole Seeding of the Spiral Galaxy NGC 4424 via an Infalling Star Cluster
- Quashing a suspected selection bias in galaxy samples having dynamically-measured supermassive black holes
- Too big to be real? No depleted core in Holm 15A
- The size--mass and other structural parameter () relations for local bulges/spheroids from multicomponent decompositions
- Running Late: Testing Delayed Supermassive Black Hole Growth Models Against the Quasar Luminosity Function
- Photoionization Modelling of the Giant Broad-Line Region in NGC 3998
- Imaging and photometric studies of NGC 1316 (Fornax A) using Astrosat/UVIT
- Star-forming S0 Galaxies in SDSS-MaNGA: fading spirals or rejuvenated S0s?
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- Discovery of a Planar Black Hole Mass Scaling Relation for Spiral Galaxies
- Identification of Intermediate-mass Black Hole Candidates Among a Sample of Sd Galaxies
- Causal Discovery in Astrophysics: Unraveling Supermassive Black Hole and Galaxy Coevolution
- Physical Processes Behind the Co-Evolution of Halos, Galaxies and Supermassive Black Holes in the IllustrisTNG Simulation
- Elliptical (E) and ellicular (ES) galaxies in the M_bh-M_*,sph diagram, and a merger-driven explanation for the origin of ES galaxies, anti-truncated stellar discs in lenticular galaxies, and the Sersicification of E galaxy light profiles