A low-luminosity type-1 QSO sample: II. Tracing circumnuclear star formation in HE 1029-1831 with SINFONI
arXiv:1412.2069 · doi:10.1051/0004-6361/201425261
Abstract
Circumnuclear star formation and AGN feedback is believed to play a critical role in the context of galaxy evolution. The low-luminosity QSO (LLQSO) sample that contains 99 of the closest AGN with redshift z<=0.06 fills the gap between the local AGN population and high-redshift QSOs that is essential to understand the AGN evolution with redshift. In this paper, we present the results of near-infrared H+K-integral field spectroscopy of the inner kiloparsecs of the LLQSO HE 1029-1831 with SINFONI. Line maps show that ionized hydrogen gas is located in spiral arms within the stellar bar and in a circumnuclear ring. Line fluxes and diagnostic line ratios indicate recent or ongoing star formation in the circumnuclear region and the presence of young and intermediate-age stellar populations in the bulge. In particular, we find traces of an intense starburst in the circumnuclear region that has begun around 100 Myr ago but has declined to a fraction of the maximum intensity now. We estimate the dynamical bulge mass and find that the galaxy follows published M_BH-M_bulge relations. However, bulge-disk decomposition of the K-band image with BUDDA reveals that HE 1029-1831 does not follow the M_BH-L_bulge relations of inactive galaxies. We conclude that the deviation from M_BH-L_bulge relations of inactive galaxies in this source is rather caused by young stellar populations and not by an undermassive black hole.
arXiv comment16 pages, 11 figures, submitted to A&A, comments welcome
References in corpus (87)
- The Global Schmidt Law in Star Forming Galaxies
- Unified Schemes for Radio-Loud Active Galactic Nuclei
- A Fundamental Relation Between Supermassive Black Holes and Their Host Galaxies
- Coevolution (Or Not) of Supermassive Black Holes and Host Galaxies
- Starburst99: Synthesis Models for Galaxies with Active Star Formation
- The Demography of Massive Dark Objects in Galaxy Centres
- Parametric Recovery of Line-of-Sight Velocity Distributions from Absorption-Line Spectra of Galaxies via Penalized Likelihood
- Reverberation Measurements for 17 Quasars and the Size-Mass-Luminosity Relations in Active Galactic Nuclei
- Secular Evolution and the Formation of Pseudobulges in Disk Galaxies
- The Relation between Black Hole Mass, Bulge Mass, and Near-Infrared Luminosity
- On the Black Hole Mass - Bulge Mass Relation
- The M-sigma and M-L Relations in Galactic Bulges and Determinations of their Intrinsic Scatter
- The SAURON project - IV. The mass-to-light ratio, the virial mass estimator and the fundamental plane of elliptical and lenticular galaxies
- An Observational Determination of the Bolometric Quasar Luminosity Function
- AGN Black Hole Masses and Bolometric Luminosities
- On the shape of the light profiles of early-type galaxies
- The Radius-Luminosity Relationship for Active Galactic Nuclei: The Effect of Host-Galaxy Starlight on Luminosity Measurements II. The Full Sample of Reverberation-Mapped AGNs
- Structural Properties of Pseudo-Bulges, Classical Bulges and Elliptical Galaxies: an SDSS Perspective
- Optimization of Starburst99 for Intermediate-Age and Old Stellar Populations
- A Close Look at Star Formation around Active Galactic Nuclei
- Reddening and Star Formation in Starburst Galaxies
- An expanded M_bh-sigma diagram, and a new calibration of active galactic nuclei masses
- The Effects of Stellar Rotation. II. A Comprehensive Set of Starburst99 Models
- The Wide Field Spectrograph (WiFeS)
- A Library of Theoretical Ultraviolet Spectra of Massive, Hot Stars for Evolutionary Synthesis
- Outflows from AGN: Kinematics of the Narrow-Line and Coronal-Line Regions in Seyfert Galaxies
- The star formation history of Seyfert 2 nuclei
- The (black hole mass)-(host spheroid luminosity) relation at high and low masses, the quadratic growth of black holes, and intermediate-mass black hole candidates
- Supermassive black holes do not correlate with galaxy disks or pseudobulges
- The Wide Field Spectrograph (WiFeS): Performance and Data Reduction
- A log-quadratic relation for predicting supermassive black hole masses from the host bulge Sersic index
- The Star-Forming Torus and Stellar Dynamical Black Hole Mass in the Seyfert 1 Nucleus of NGC3227
- BUDDA: A New Two-Dimensional Bulge/Disk Decomposition Code for Detailed Structural Analysis of Galaxies
- The Spitzer/IRAC view of black hole - bulge scaling relations
- Image Decomposition of Barred Galaxies and AGN Hosts
- Molecular Gas in NUclei of GAlaxies (NUGA): IV. Gravitational Torques and AGN Feeding
- Mapping of the molecular gas inflow towards the Seyfert nucleus of NGC4051 using Gemini NIFS
- Do quiescent and active galaxies have different M_BH-sigma relations?
- The Relationship Between Black Hole Mass and Velocity Dispersion in Seyfert 1 Galaxies
- Feeding versus Feedback in NGC 4151 probed with Gemini NIFS. I. Excitation
- Low redshift AGN in the Hamburg/ESO Survey: II. The active black hole mass function and the distribution function of Eddington ratios
- The Supermassive Black Hole Mass - Spheroid Stellar Mass Relation for Sérsic and Core-Sérsic Galaxies
- Molecular Hydrogen and [FeII] in Active Galactic Nuclei
- Molecular Gas in NUclei of GAlaxies (NUGA) I.The counter-rotating LINER NGC4826
- Dust and Nebular Emission. I. Models for Normal Galaxies
- A SINFONI view of Galaxy Centers: Morphology and Kinematics of five Nuclear Star Formation Rings
- A Near Infrared Spectroscopic Survey of LINER Galaxies
- A Local Baseline of the Black Hole Mass Scaling Relations for Active Galaxies. I. Methodology and Results of Pilot Study
- Quasar host galaxy star formation activity from multicolour data
- SINFONI adaptive optics integral field spectroscopy of the Circinus Galaxy
- The properties of the extended warm ionised gas around low-redshift QSOs and the lack of extended high-velocity outflows
- Integral field spectroscopy of nearby QSOs: I. ENLR size-luminosity relation, ongoing star formation & resolved gas-phase metallicities
- The Gemini spectral library of near-IR late type stellar templates and its application for velocity dispersion measurements
- AGN-Starburst connection in NGC7582: Gemini near-infrared spectrograph integral field unit observations
- Molecular Hydrogen and [Fe II] in Active Galactic Nuclei III: LINERS and Star Forming Galaxies
- The Origin of the Intrinsic Scatter in the Relation Between Black Hole Mass and Bulge Luminosity for Nearby Active Galaxies
- Molecular gas in the centre of nearby galaxies from VLT/SINFONI integral field spectroscopy - I. Morphology and mass inventory
- Warm and Cold Molecular Gas in Galaxies
- The [FeII]1.644micron emission in M82 and NGC253: Is it a measure of the supernova rate?
- Molecular gas in nearby low-luminosity QSO host galaxies
- Compact molecular disc and ionized gas outflows within 350 pc of the active nucleus of Mrk 1066
- Feeding and feedback in the active nucleus of Mrk 1157 probed with Gemini Near-Infrared Integral-Field Spectrograph
- Near-IR Spectra of Red Supergiants and Giants. I- Models with Solar and with Mixing-Induced Surface Abundance Ratios
- Gemini Near Infrared Integral Field Spectroscopy of the Narrow-Line Region of ESO428-G14: kinematics, excitation and the role of the radio jet
- Molecular Hydrogen Excitation in Ultraluminous Infrared Galaxies
- Supermassive Black Holes and Their Host Galaxies - II. The correlation with near-infrared luminosity revisited
- New Estimators of Black Hole Mass in Active Galactic Nuclei with Hydrogen Paschen Lines
- The near-IR - L and - n relations
- Molecular Hydrogen Excitation around Active Galactic Nuclei
- Molecular Gas in NUclei of GAlaxies (NUGA): II. The Ringed LINER NGC7217
- Feeding Versus Feedback in NGC1068 probed with Gemini NIFS. I. Excitation
- The supermassive black hole mass - Sérsic index relations for bulges and elliptical galaxies
- NUclei of GAlaxies: V. Radio emission in 7 NUGA sources
- The circumnuclear environment of NGC613: a nuclear starburst caught in the act?
- Low redshift AGN in the Hamburg/ESO Survey: I. The local AGN luminosity function
- A low-luminosity type-1 QSO sample: I. Overluminous host spheroidals or undermassive black holes?
- X-rays as dominant excitation mechanism of [Fe ii] and H2 emission lines in active galaxies
- Resolving the coronal line region of NGC1068 with near-infrared integral field spectroscopy
- Modeling Tracers of Young Stellar Population Age in Star-Forming Galaxies
- The RASS--6dFGS catalogue: a sample of X-ray selected AGN from the 6dF Galaxy Survey
- Near-Infrared Integral Field Spectroscopy of Star-Forming Galaxies
- Nearby AGN and their hosts in the near infrared
- Mrk 609: resolving the circum-nuclear structure with near-infrared integral field spectroscopy
- Differences between CO- and calcium triplet-derived velocity dispersions in spiral galaxies: evidence for central star formation?
- Is IRAS 01072+4954 a True-Seyfert 2? Hints from Near Infrared Integral Field Spectroscopy
- ALMA backed NIR high resolution integral field spectroscopy of the NUGA galaxy NGC 1433
- Barred CO emission in HE1029-1831
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- The nuclear gas disk of NGC 1566 dissected by SINFONI and ALMA
- The Close AGN Reference Survey (CARS): No obvious signature of AGN feedback on star formation, but subtle trends
- Near-infrared observations of star formation and gas flows in the NUGA galaxy NGC 1365
- Star formation and gas flows in the centre of the NUGA galaxy NGC 1808 observed with SINFONI
- The effect of the environment-dependent stellar initial mass function on the photometric properties of star-forming galaxies
- A low-luminosity type-1 QSO sample. V. Overluminous host spheroids and their excitation mechanisms
- A low-luminosity type-1 QSO sample: IV. Molecular gas contents and conditions of star formation in three nearby Seyfert galaxies
- A low-luminosity type-1 QSO sample; III. Optical spectroscopic properties and activity classification
- The Close AGN Reference Survey (CARS): SOFIA detects spatially-resolved [CII] emission in the luminous AGN HE0433-1028
- Correlations between Supermassive Black Holes and their Hosts in Active Galaxies