Triggered or Self-Regulated Star Formation within Intermediate Redshift Luminous Infrared Galaxies (I). Morphologies and Spatially Resolved Spectral Energy Distributions
arXiv:0801.1135 · doi:10.1088/0004-6256/135/4/1207
Abstract
We imaged a set of 15 intermediate redshift (z~0.8) luminous infrared galaxies (LIRGs) with the Keck Laser Guide Star (LGS) AO facility. These galaxies were selected from the GOODS-S field, allowing us to combine the high spatial resolution HST optical (B, V, i, and z-bands) images with our near-infrared (K'-band) images to study the LIRG morphologies and spatially resolved spectral energy distributions (SEDs). Two thirds of the LIRGs are disk galaxies, with only one third showing some evidence for interactions, minor, or major mergers. In contrast with local LIRG disks (which are primarily barred systems), only 10% of the LIRG disks in our sample contain a prominent bar. While the optical bands tend to show significant point-like substructure, indicating distributed star formation, the AO K-band images tend to be smooth. The SEDs of the LIRGs are consistent with distributed dusty star formation, as exhibited by optical to IR colors redder than allowed by old stellar populations alone. This effect is most pronounced in the galaxy cores, possibly indicating central star formation. We also observed a set of 11 intermediate redshift comparison galaxies, selected to be non-ellipticals with apparent K-band magnitudes comparable to the LIRGs. The "normal" (non-LIRG) systems tended to have lower optical luminosity, lower stellar mass, and more irregular morphology than the LIRGs. Half of the "normal" galaxies have SEDs consistent with intermediate aged stellar populations and minimal dust. The other half show evidence for some dusty star formation, usually concentrated in their cores. Our work suggests that the LIRG disk galaxies are similar to large disk systems today, undergoing self regulated star formation, only at 10 - 20 times higher rates. (Abridged)
Accepted for Publication in AJ. 27 pages, 21 figures, 3 tables
References in corpus (27)
- Stellar population synthesis at the resolution of 2003
- The Cosmic Evolution Survey (COSMOS) -- Overview
- A Simple Model for the Absorption of Starlight by Dust in Galaxies
- The Great Observatories Origins Deep Survey: Initial Results From Optical and Near-Infrared Imaging
- The reversal of the star formation-density relation in the distant universe
- Infrared luminosity functions from the Chandra Deep Field South : the Spitzer view on the history of dusty star formation at 0<z<1
- The Chandra Deep Field South: Optical Spectroscopy I
- Towards an understanding of the rapid decline of the cosmic star formation rate
- The Evolution of Galaxy Mergers and Morphology at z<1.2 in the Extended Groth Strip
- GEMS: Galaxy Evolution from Morphologies and SEDs
- A catalogue of the Chandra Deep Field South with multi-colour classification and photometric redshifts from COMBO-17
- Evolution of the Bar Fraction in COSMOS: Quantifying the Assembly of the Hubble Sequence
- The DEEP2 Galaxy Redshift Survey: The Galaxy Luminosity Function to z ~ 1
- The Team Keck Treasury Redshift Survey of the GOODS-North Field
- Did most present-day spirals form during the last 8 Gyrs? A formation history with violent episodes revealed by panchromatic observations
- The Nature of Compact Galaxies in the Hubble Deep Field (II): Spectroscopic Properties and Implications for the Evolution of the Star Formation Rate Density of the Universe
- The Great Observatories Origins Deep Survey VLT/FORS2 Spectroscopy in the GOODS-South Field: Part II
- Optical Morphology Evolution of Infrared Luminous Galaxies in GOODS-N
- Luminous Infrared Galaxies in the Local Universe
- VLA Observations of Ultraluminous IRAS Galaxies: Active Nuclei or Starbursts?
- A Study of the Distribution of Star-Forming Regions in Luminous Infrared Galaxies by Means of H Imaging Observations
- HST/WFPC2 morphologies and bar structures of field galaxies at 0.4<z<1
- Merging Galaxies in Goods-s: First Extragalactic Results from Keck Laser Adaptive Optics
- Radius Dependent Luminosity Evolution of Blue Galaxies in GOODS-N
- Sample of minor merger of galaxies: Optical CCD surface photometry and HII region propertie
- Red Supergiants in the Disk of M81: Tracing the Spatial Distribution of Star Formation 25 Million Years in the Past
- Rest-Frame R-band Lightcurve of a z~1.3 Supernova Obtained with Keck Laser Adaptive Optics
Cited by in corpus (27)
- The Persistence of Cool Galactic Winds in High Stellar Mass Galaxies Between z~1.4 and ~1
- Far-infrared Fine-Structure Line Diagnostics of Ultraluminous Infrared Galaxies
- An HST/WFC3-IR Morphological Survey of Galaxies at z = 1.5-3.6: I. Survey Description and Morphological Properties of Star Forming Galaxies
- Spectral Energy Distributions of Local Luminous And Ultraluminous Infrared Galaxies
- Galaxy Mergers and Dark Matter Halo Mergers in LCDM: Mass, Redshift, and Mass-Ratio Dependence
- Galaxy pairs in the Sloan digital sky survey - VII: The merger -- luminous infra-red galaxy connection
- Specific star-formation and the relation to stellar mass from 0<z<2 as seen in the far-infrared at 70 and 160mu
- Compton Thick AGN in the XMM-COSMOS survey
- The Inner Kiloparsec of Mrk 273 with Keck Adaptive Optics
- Polycyclic aromatic hydrocarbon (PAH) luminous galaxies at z~1
- Role of Galaxy Mergers in Cosmic Star Formation History
- A comparison of the morphological properties between local and z~1 infrared luminous galaxies. Are local and high-z (U)LIRGs different?
- An Evolutionary Paradigm for Dusty Active Galaxies at Low Redshift
- High Redshift Dust Obscured Galaxies, A Morphology-SED Connection Revealed by Keck Adaptive Optics
- Black Hole Masses and Star Formation Rates of z >1 Dust Obscured Galaxies (DOGs): Results from Keck OSIRIS Integral Field Spectroscopy
- Morphologies of High Redshift, Dust Obscured Galaxies from Keck Laser Guide Star Adaptive Optics
- Active Disk Building in a local HI-Massive LIRG: The Synergy between Gas, Dust, and Star Formation
- [Ultra] Luminous Infrared Galaxies selected at 90 m in the AKARI deep field: a study of AGN types contributing to their infrared emission
- The Asymptotic Giant Branch and the Tip of the Red Giant Branch as Probes of Star Formation History: The Nearby Dwarf Irregular Galaxy KKH 98
- MOIRCS Deep Survey. VII: NIR Morphologies of Star-forming Galaxies at Redshift z~1
- Spatially Resolved Stellar Populations of Eight GOODS-South AGN at z~1
- The hidden HI-massive LIRG HIZOA J0836-43: Inside-out galaxy formation
- Kinematics of an isolated galaxy, CIG 993
- LGS AO Science Impact: Present and Future Perspectives
- Dusty Universe viewed by AKARI far infrared detector
- A multiwavelength study of the IRAS Deep Survey galaxy sample III. Spectral classification and dynamical properties
- Ultraviolet-to-far-infra-red self-consistent analysis of the stellar populations of massive starburst galaxies at intermediate redshifts