Thick Disks in the Hubble Space Telescope Frontier Fields
arXiv:1709.00114 · doi:10.3847/1538-4357/aa88d4
Abstract
Thick disk evolution is studied using edge-on galaxies in two Hubble Space Telescope Frontier Field Parallels. The galaxies were separated into 72 clumpy types and 35 spiral types with bulges. Perpendicular light profiles in F435W, F606W and F814W (B, V and I) passbands were measured at 1 pixel intervals along the major axes and fitted to sech^2 functions convolved with the instrument line spread function (LSF). The LSF was determined from the average point spread function (PSF) of ~20 stars in each passband and field, convolved with a line of uniform brightness to simulate disk blurring. A spread function for a clumpy disk was also used for comparison. The resulting scale heights were found to be proportional to galactic mass, with the average height for a 10^9.5-10^10.5 Msun galaxy at z=1.5-2.5 equal to 0.63+-0.24 kpc. This value is probably the result of a blend between thin and thick disk components that cannot be resolved. Evidence for such two-component structure is present in an inverse correlation between height and midplane surface brightness. Models suggest that the thick disk is observed best between the clumps, and there the average scale height is 1.06+-0.43 kpc for the same mass and redshift. A 0.63+-0.68 mag V-I color differential with height is also evidence for a mixture of thin and thick components.
arXiv comment11 pages, 19 figures, accepted by ApJ
References in corpus (45)
- Stellar population synthesis at the resolution of 2003
- The Average Star Formation Histories of Galaxies in Dark Matter Halos from z=0-8
- The SINS survey: SINFONI Integral Field Spectroscopy of z ~ 2 Star-forming Galaxies
- The Frontier Fields: Survey Design
- Chemical Cartography with APOGEE: Metallicity Distribution Functions and the Chemical Structure of the Milky Way Disk
- The spatial structure of mono-abundance sub-populations of the Milky Way disk
- The thick disks of spiral galaxies as relics from gas-rich, turbulent, clumpy disks at high redshift
- Structural Parameters of Thin and Thick Disks in Edge-On Disk Galaxies
- The Milky Way has no thick disk
- Inside Out and Upside Down: Tracing the Assembly of a Simulated Disk Galaxy Using Mono-Age Stellar Populations
- The Epoch of Disk Settling: z~1 to Now
- A First Constraint on the Thick Disk Scale Length: Differential Radial Abundances in K Giants at Galactocentric Radii 4, 8, and 12 kpc
- Formation and Evolution of the Disk System of the Milky Way: [alpha/Fe] Ratios and Kinematics of the SEGUE G-Dwarf Sample
- A Structural and Dynamical Study of Late-Type, Edge-On Galaxies: II. Vertical Color Gradients and the Detection of Ubiquitous Thick Disks
- On the Formation of Galactic Thick Disks
- Rigging dark halos: why is hierarchical galaxy formation consistent with the inside-out build-up of thin discs?
- Observations of Thick Disks in the Hubble Space Telescope Ultra Deep Field
- Constraining the thick disc formation scenario of the Milky Way
- Tracing the Galactic thick disk to Solar metallicities
- The Origin of the Light Distribution in Spiral Galaxies
- Balance among gravitational instability, star formation, and accretion determines the structure and evolution of disk galaxies
- Thick disks of edge-on galaxies seen through the Spitzer Survey of Stellar Structure in Galaxies (S4G): Lair of missing baryons?
- A Short Scale Length for the α-Enhanced Thick Disk of the Milky Way: Evidence from Low-Latitude SEGUE Data
- MaGICC Thick Disk I: Comparing a Simulated Disk Formed with Stellar Feedback to the Milky Way
- Vertical scaleheights in a gravitationally coupled, three-component Galactic disk
- Forming disk galaxies in wet major mergers. I. Three fiducial examples
- Accretion-Driven Turbulence and the Transition to Global Instability in Young Galaxy Disks
- The effect of radial migration on galactic disks
- The ASTRODEEP Frontier Fields Catalogues: II - Photometric redshifts and rest-frame properties in Abell-2744 and MACS-J0416
- The vertical motions of mono-abundance sub-populations in the Milky Way disk
- The ASTRODEEP Frontier Fields Catalogues: I - Multiwavelength photometry of Abell-2744 and MACS-J0416
- Dissecting simulated disc galaxies II: the age-velocity relation
- The Kinematics of Thick Disks in Nine External Galaxies
- Idealized models for galactic disk formation and evolution in 'realistic' LambdaCDM haloes
- Lick Indices in the Thin and Thick Disks of Edge-On Disk Galaxies
- A Star Formation Law for Dwarf Irregular Galaxies
- The Onset of Spiral Structure in the Universe
- The influence of diffuse scattered light II. Observations of galaxy haloes and thick discs and hosts of BCGs
- The quiescent phase of galactic disc growth
- Chemo-orbital evidence from SDSS/SEGUE G-type dwarf stars for a mixed origin of the Milky Way's thick disk
- Evidence for the concurrent growth of thick discs and central mass concentrations from SG imaging
- The Diversity of Thick Galactic Discs
- A monolithic collapse origin for the thin/thick disc structure of ESO 243-49
- The imprint of radial migration on the vertical structure of galaxy disks
- Properties of thick discs formed in clumpy galaxies
Cited by in corpus (36)
- The SINS/zC-SINF survey of z~2 galaxy kinematics: SINFONI adaptive optics-assisted data and kiloparsec-scale emission line properties
- The Fornax 3D project: unveiling the thick disk origin in FCC 170: signs of accretion?
- The bursty origin of the Milky Way thick disc
- Systematic difference between ionized and molecular gas velocity dispersion in disks and local analogues
- Born this way: thin disc, thick disc, and isotropic spheroid formation in FIRE-2 Milky-Way-mass galaxy simulations
- Stars behind bars I: The Milky Way's central stellar populations
- The KMOS Survey: Investigating the Origin of the Elevated Electron Densities in Star-Forming Galaxies at
- Kinematic decomposition of IllustrisTNG disk galaxies: morphology and relation with morphological structures
- Identifying kinematic structures in simulated galaxies using unsupervised machine learning
- Geometric properties of galactic discs with clumpy episodes
- Introducing galactic structure finder: the multiple stellar kinematic structures of a simulated Milky Way mass galaxy
- NIHAO XVI: The properties and evolution of kinematically selected discs, bulges and stellar haloes
- Two Thresholds for Globular Cluster Formation and their Dominance of Star Formation in the Early-Universe
- The most ancient spiral galaxy: a 2.6-Gyr-old disk with a tranquil velocity field
- MusE GAs FLOw and Wind (MEGAFLOW) IV: A two sightline tomography of a galactic wind
- Molecular gas cloud properties at revealed by the superb angular resolution achieved with ALMA and gravitational lensing
- Towards sub-kpc scale kinematics of molecular and ionized gas of star-forming galaxies at
- A first estimate of the Milky Way dark matter halo spin
- NGC 7469 as seen by MEGARA: new results from high-resolution IFU spectroscopy
- Evolution of Disc Thickness in Simulated High-Redshift Galaxies
- The structure of the Milky Way based on unWISE 3.4m integrated photometry
- On the Flaring of Thick Disc of Galaxies: Insights from Simulations
- Little Blue Dots in the Hubble Space Telescope Frontier Fields: Precursors to Globular Clusters?
- The Connection between Mergers and AGN Activity in Simulated and Observed Massive Galaxies
- Structure and stability of high-redshift galaxies in cosmological simulations
- On the Impact of Inclination-Dependent Attenuation on Derived Star Formation Histories: Results from Disk Galaxies in the Great Observatories Origins Deep Survey Fields
- The Panchromatic Hubble Andromeda Treasury XX: The Disk of M31 is Thick
- The Extraplanar Type II Supernova ASASSN-14jb in the Nearby Edge-on Galaxy ESO 467-G051
- The imprint of the thick stellar disc in the mid-plane of three early-type edge-on galaxies in the Fornax cluster
- Linking star formation thresholds and truncations in the thin and thick disks of the low-mass galaxy UGC 7321
- Insights into the Formation and Evolution History of the Galactic Disk System
- Damped Lyman- absorbers and atomic hydrogen in galaxies: the view of the GAEA model
- Rediscovering the Milky Way with orbit superposition approach and APOGEE data II. Chrono-chemo-kinematics of the disc
- Orbital Migration through Atmospheric Mass Loss
- Through Thick and Thin: The Cosmic Evolution of Disk Scale Height
- Magnetising galaxies with cold inflows