Formation of S0 galaxies through mergers. Evolution in the Tully-Fisher relation since $z\sim 1$

Abstract

(Abridged version) We explore whether a scenario that combines an origin by mergers at $z\sim$1.8-1.5 with a subsequent passive evolution of the resulting S0 remnants since $z\sim$0.8-1 is compatible with observational data of S0s in the Tully-Fisher relation (TFR). We studied a set of major and minor merger experiments from the GalMer database that generate massive S0 remnants. We analysed the location of these remnants in the photometric and stellar TFRs assuming that they correspond to $z\sim 0.8$ galaxies. We then estimated their evolution in these planes over the last 7 Gyr. The results were compared with data of real S0s and spirals at different redshifts. We also tested how the use of Vcirc or Vrot,max affects the results. We found that just after $\sim$1-2 Gyr of coalescence, major mergers generate S0 remnants that are outliers of the local photometric and stellar TFRs at $z\sim 0.8$. After $\sim$4-7 Gyr of passive evolution in isolation, the S0 remnants move towards the local TFR, although the initial scatter among them persists. This scatter is sensitive to the indicator used for the rotation velocity: Vcirc values yield a lower scatter than when Vrot,max values are considered instead. In the planes involving Vrot,max, a clear segregation of the S0 remnants in terms of the spin-orbit coupling of the model is observed, in which the remnants of retrograde encounters overlap with local S0s hosting counter-rotating discs. The location of the S0 remnants at $z\sim 0$ agrees well with the observed distribution of local S0 galaxies in the ${\sigma }_0$-$M_K$, Vcirc-${\sigma }_0$ and Vrot,max-${\sigma }_0$ planes. Thus, massive S0 galaxies may have been formed through major mergers that occurred at high redshift and have later evolved towards the local TFR through passive evolution in relative isolation, a mechanism that would also contribute to the scatter observed in this relation.

19 pages, 15 figures. Accepted for publication in A&A

References in corpus (31)

• HyperLEDA. III. The catalogue of extragalactic distances
• From rings to bulges: evidence for rapid secular galaxy evolution at z~2 from integral field spectroscopy in the SINS survey
• Strangulation as the primary mechanism for shutting down star formation in galaxies
• Riding the Spiral Waves: Implications of Stellar Migration for the Properties of Galactic Disks
• The SAURON project - VII. Integral-field absorption and emission-line kinematics of 24 spiral galaxy bulges
• The SAURON project - VIII. OASIS/CFHT integral-field spectroscopy of elliptical and lenticular galaxy centres
• The metallicity gradient of M 33: chemical abundances of HII regions
• The effect of radial migration on galactic disks
• The Tully-Fisher relation for S0 galaxies
• The formation of stellar nuclear discs in bar-induced gas inflows
• Galactic abundance gradients from Cepheids : On the iron abundance gradient around 10-12 kpc
• Growth of galactic bulges by mergers. II. Low-density satellites
• Bars, ovals and lenses in early-type disk galaxies: probes of galaxy evolution
• Formation of S0 galaxies through mergers. Bulge-disc structural coupling resulting from major mergers
• Formation of S0 galaxies through mergers. V. Antitruncated stellar discs resulting from major mergers
• Building gas rings and rejuvenating S0 galaxies through minor mergers
• 2D velocity fields of simulated interacting disc galaxies
• Properties of dust in early-type galaxies
• Testing the nature of S0 galaxies using planetary nebula kinematics in NGC 1023
• The Planetary Nebula Spectrograph survey of S0 galaxy kinematics. Data and Overview
• A New Channel for the Formation of Kinematically Decoupled Cores in Early-type galaxies
• The effects of ram-pressure stripping on the internal kinematics of simulated spiral galaxies
• Line-of-sight velocity distributions of elliptical galaxies from collisionless mergers
• Internal kinematics of modelled interacting disc galaxies
• Evolution induced by dry minor mergers onto fast-rotator S0 galaxies
• The slowing down of galaxy disks in dissipationless minor mergers
• An investigation of star formation and dust attenuation in major mergers using ultraviolet and infrared data
• Old stellar counter-rotating components in early-type galaxies from elliptical-spiral mergers
• Ionized gas disks in elliptical and S0 galaxies at $z<1$
• Evolution of the optical Tully-Fisher relation up to z=1.3
• The Tully-Fisher relation of galaxies at z~0.85 in the DEEP2 survey

Cited by in corpus (32)

• Combining Stellar Populations with Orbit-Superposition Dynamical Modelling - the Formation History of the Lenticular Galaxy NGC 3115
• The two formation pathways of S0 galaxies
• The SAMI Galaxy Survey: A Range in S0 Properties Indicating Multiple Formation Pathways
• The Fornax3D project: Assembly histories of lenticular galaxies from a combined dynamical and population orbital analysis
• The origin of metal-poor stars on prograde disk orbits in FIRE simulations of Milky Way-mass galaxies
• Galaxy interactions in IllustrisTNG-100, I: The power and limitations of visual identification
• Formation of S0s in extreme environments I: clues from kinematics and stellar populations
• The SLUGGS survey: combining stars, globular clusters and planetary nebulae to understand the assembly history of early-type galaxies from their large radii kinematics
• Double-peak emission line galaxies in the SDSS catalogue. A minor merger sequence
• The SAMI Galaxy Survey: bulge and disk stellar population properties in cluster galaxies
• The galaxy morphology-density relation in the EAGLE simulation
• SH$\alpha$DE: Survey description and mass-kinematics scaling relations for dwarf galaxies
• The relation between morphology, star formation history, and environment in local universe galaxies
• Evolution of compact groups from intermediate to final stages: A case study of the HI content of HCG 16
• BUDDI-MaNGA II: The Star-Formation Histories of Bulges and Discs of S0s
• A Virgo Environmental Survey Tracing Ionised Gas Emission (VESTIGE).XII. Ionised gas emission in the inner regions of lenticular galaxies
• The local universe in the era of large surveys. I. Spectral classification of S0 galaxies
• The SAMI Galaxy Survey: The role of disc fading and progenitor bias in kinematic transitions
• Formation of S0s in extreme environments III: the role of environment in the formation pathways
• Recovering the origins of the lenticular galaxy NGC 3115 using multi-band imaging
• Connecting galaxy structure and star formation: the role of environment in formation of S0 galaxies
• Evolution of the anti-truncated stellar profiles of S0 galaxies since $z=0.6$ in the SHARDS survey: I - Sample and Methods
• The redshift evolution of the S0 fraction for $z<1$ in COSMOS
• Massive Red Spiral Galaxies in SDSS-IV MaNGA Survey
• The complex globular cluster system of the S0 galaxy NGC 4382 in the outskirts of the Virgo Cluster
• The origin of star-forming rings in S0 galaxies
• The physical properties of S0 galaxy PGC 26218: the origin of starburst and star formation
• A MaNGA view of isolated galaxy mergers in the star-forming Main Sequence
• The present-day globular cluster kinematics of lenticular galaxies from the E-MOSAICS simulations and their relation to the galaxy assembly histories
• The distribution of lenticular galaxies in the phase space of present-day galaxy cluster regions
• Stellar Populations of Spectroscopically Decomposed Bulge-Disk for S0 Galaxies from the CALIFA survey
• Star-forming S0 Galaxies in SDSS-MaNGA: fading spirals or rejuvenated S0s?