Photometric properties of classical bulge and pseudo-bulge galaxies at $0.5\le z<1.0$

Abstract

We compare the photometric properties and specific star formation rate (sSFR) of classical and pseudo-bulge galaxies with $M_{\ast }\ge 10^{9.5}{\mathrm{M}}_{\odot }$ at $0.5\le z<1.0$, selected from all five CANDELS fields. We also compare these properties of bulge galaxies at lower redshift selected from MaNGA survey (Hu et al. 2024). This paper aims to study the properties of galaxies with classical and pseudo-bulges at intermediate redshift, to compare the differences between different bulge types, and to understand the evolution of bulges with redshift. Galaxies are classified into classical bulge and pseudo-bulge samples according to the S$\acute{\mathrm{e}}$rsic index n of the bulge component based on results of two-component decomposition of galaxies, as well as the position of bulges on the Kormendy diagram. For the 105 classical bulge and 86 pseudo-bulge galaxies selected, we compare their size, luminosity, and sSFR of various components. At given stellar mass, most classical bulge galaxies have smaller effective radii, larger $B/T$, brighter and relatively larger bulges, and less active star formation than pseudo-bulge galaxies. Besides, the two types of galaxies have larger differences in sSFR at large radii than at the central region at both low and mid-redshifts. The differences between properties of the two types of bulge galaxies are in general smaller at mid-redshift than at low redshift, indicating that they are evolving to more distinct populations towards the local universe. Bulge type is correlated with the properties of their outer disks, and the correlation is already present at redshift as high as $0.5<z<1$.

arXiv comment9 pages, 7 figures, 1 table. Submitted to A&A

References in corpus (63)

• Stellar population synthesis at the resolution of 2003
• Galactic Stellar and Substellar Initial Mass Function
• Star Formation in Galaxies Along the Hubble Sequence
• The Dust Content and Opacity of Actively Star-Forming Galaxies
• Detailed Structural Decomposition of Galaxy Images
• Parametric Recovery of Line-of-Sight Velocity Distributions from Absorption-Line Spectra of Galaxies via Penalized Likelihood
• CANDELS: The Cosmic Assembly Near-infrared Deep Extragalactic Legacy Survey
• CANDELS: The Cosmic Assembly Near-infrared Deep Extragalactic Legacy Survey - The Hubble Space Telescope Observations, Imaging Data Products and Mosaics
• The James Webb Space Telescope
• Secular Evolution and the Formation of Pseudobulges in Disk Galaxies
• Overview of the SDSS-IV MaNGA Survey: Mapping Nearby Galaxies at Apache Point Observatory
• Improving the full spectrum fitting method: accurate convolution with Gauss-Hermite functions
• UniverseMachine: The Correlation between Galaxy Growth and Dark Matter Halo Assembly from z=0-10
• An ultra-deep near-infrared spectrum of a compact quiescent galaxy at z=2.2
• From rings to bulges: evidence for rapid secular galaxy evolution at z~2 from integral field spectroscopy in the SINS survey
• Structural Properties of Pseudo-Bulges, Classical Bulges and Elliptical Galaxies: an SDSS Perspective
• Structural Parameters of Galaxies in CANDELS
• CANDELS Multi-wavelength Catalogs: Source Detection and Photometry in the GOODS-South Field
• Mergers and Bulge Formation in Lambda-CDM: Which Mergers Matter?
• EMERGE - An empirical model for the formation of galaxies since $z\sim 10$
• Early Evolution of Disk Galaxies : Formation of Bulges in Clumpy Young Galactic Disks
• Bulge Formation by the Coalescence of Giant Clumps in Primordial Disk Galaxies
• CANDELS Multiwavelength catalogs: Source Identification and Photometry in the CANDELS UKIDSS Ultra-Deep Survey Field
• Bulgeless Giant Galaxies Challenge our Picture of Galaxy Formation by Hierarchical Clustering
• Did most present-day spirals form during the last 8 Gyrs? A formation history with violent episodes revealed by panchromatic observations
• Bulges Of Nearby Galaxies With Spitzer: Scaling Relations in Pseudobulges and Classical Bulges
• CANDELS Multiwavelength Catalogs: Source Identification and Photometry in the CANDELS Extended Groth Strip
• The CANDELS/SHARDS multi-wavelength catalog in GOODS-N: Photometry, Photometric Redshifts, Stellar Masses, Emission line fluxes and Star Formation Rates
• Growth of Galactic Bulges by Mergers: I. Dense Satellites
• Double Bars, Inner Disks, and Nuclear Rings in Early-Type Disk Galaxies
• CANDELS Multiwavelength Catalogs: Source Identification and Photometry in the CANDELS COSMOS Survey Field
• Demographics of Bulge Types within 11 Mpc and Implications for Galaxy Evolution
• Radial Mixing in Galactic Disks: The Effects of Disk Structure and Satellite Bombardment
• SDSS-IV DR17: Final Release of MaNGA PyMorph Photometric and Deep Learning Morphological Catalogs
• A Connection Between Bulge Properties and the Bimodality of Galaxies
• An observer's view of simulated galaxies: disc-to-total ratios, bars, and (pseudo-)bulges
• Structure and star formation in disk galaxies III. Nuclear and circumnuclear H alpha emission
• Demographics of Star-forming Galaxies since $z\sim 2.5$. I. The $UVJ$ Diagram in CANDELS
• Kinematic Signatures of Bulges Correlate with Bulge Morphologies and Sérsic Index
• Pseudobulge Formation as a Dynamical Rather than a Secular Process
• Quantifying stellar radial migration in an N-body simulation: blurring, churning, and the outer regions of galaxy discs
• Formation of S0 galaxies through mergers: Explaining angular momentum and concentration change from spirals to S0s
• An Observational Guide to Identifying Pseudobulges and Classical Bulges in Disk Galaxies
• Bulges Of Nearby Galaxies With Spitzer: The Growth Of Pseudobulges In Disk Galaxies And Its Connection To Outer Disks
• Natures of a clump-origin bulge: a pseudobulge-like but old metal-rich bulge
• A close look at secular evolution: Boxy/peanut bulges reduce gas inflow to the central kiloparsec
• Orbits of radial migrators and non-migrators around a spiral arm in N-body simulations
• UVI colour gradients of 0.4<z<1.4 star-forming main sequence galaxies in CANDELS: dust extinction and star formation profiles
• Recovering stellar population parameters via two full-spectrum fitting algorithms in the absence of model uncertainties
• Observed properties of boxy/peanut/barlens bulges
• Recovering stellar population parameters via different population models and stellar libraries
• SDSS-IV MaNGA: Stellar M/L gradients and the M/L-colour relation in galaxies
• Evolution along the sequence of S0 Hubble types induced by dry minor mergers. II - Bulge-disk coupling in the photometric relations through merger-induced internal secular evolution
• Growth of bulges in disc galaxies since $z\sim 1$
• Most pseudo-bulges can be formed at later stages of major mergers
• Galaxy Flybys: Evolution of the Bulge, Disk, and Spiral Arms
• On the Transition of the Galaxy Quenching Mode at 0.5<z<1 in CANDELS
• Deep Extragalactic VIsible Legacy Survey (DEVILS): The emergence of bulges and decline of disk growth since $z=1$
• Correlation of structure and stellar properties of galaxies in Stripe 82
• Growth of disc-like pseudo-bulges in SDSS DR7 since z = 0.1
• The clustering of galaxies with pseudo bulge and classical bulge in the local Universe
• Bright Compact Bulges (BCBs) at intermediate redshifts
• SDSS-IV MaNGA: Stellar rotational support in disk galaxies vs. central surface density and stellar population age

Cited by in corpus (1)

• Investigating the Bulge Morphology of Dual AGN Host Galaxies from the GOTHIC survey