The distance to the Orion Nebula
arXiv:0709.0485 · doi:10.1051/0004-6361:20078247
Abstract
We have used the Very Long Baseline Array to measure the trigonometric parallax of several member stars of the Orion Nebula Cluster showing non-thermal radio emission. We have determined the distance to the cluster to be 414 +/- 7 pc. Our distance determination allows for an improved calibration of luminosities and ages of young stars. We have also measured the proper motions of four cluster stars which, when accurate radial velocities are measured, will put strong constraints on the origin of the cluster.
13 pages, 3 figures, to appear in Astronomy & Astrophyiscs
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- Encounters in the ONC - observing imprints of star-disc interactions
- Three-dimensional dust density structure of the Orion, Cygnus X,Taurus, and Perseus star-forming regions
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- Mapping young stellar populations towards Orion with Gaia DR1
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- First Science Observations with SOFIA/FORCAST: Properties of Intermediate-Luminosity Protostars and Circumstellar Disks in OMC-2
- The Small-Scale Physical Structure and Fragmentation Difference of Two Embedded Intermediate Mass Protostars in Orion
- The infrared spectrograph survey of protoplanetary disks in Orion A: I. disk properties
- First astronomical unit scale image of the GW Ori triple. Direct detection of a new stellar companion
- A non-equilibrium ortho-to-para ratio of water in the Orion PDR
- ALMA Images of the Orion Hot Core at 349 GHz
- Kompaneets Model Fitting of the Orion-Eridanus Superbubble II: Thinking Outside of Barnard's Loop
- Surface chemistry in photodissociation regions
- Small Protoplanetary Disks in the Orion Nebula Cluster and OMC1 with ALMA
- The PDR structure and kinematics around the compact HII regions S235A and S235C with [CII], [13CII], [OI] and HCO+ line profiles
- The seven sisters DANCe IV. Bayesian hierarchical model
- Earliest Stages of Protocluster Formation: Substructure and Kinematics of Starless Cores in Orion
- The structure of the Orion Nebula in the direction of Theta 1 Ori C
- A study of dynamical processes in the Orion KL region using ALMA-- Probing molecular outflow and inflow
- VLBA imaging of the 3mm SiO maser emission in the disk-wind from the massive protostellar system Orion Source I
- A VLT/NACO Study of Star Formation in the Massive Embedded Cluster RCW 38
- Nobeyama 45 m Mapping Observations toward Orion A. II. Classification of cloud structures and variation of the CO/CO abundance ratio due to far-UV Radiation
- SDSS-V Local Volume Mapper (LVM): A Glimpse into Orion
- Short- and long-term variability of young stars in the Orion Nebula Cluster and Molecular Cloud
- The Core Mass Function in the Orion Nebula Cluster Region: What Determines the Final Stellar Masses?
- Carbon radio recombination lines from gigahertz to megahertz frequencies towards Orion A
- Witnessing the fragmentation of a filament into prestellar cores in Orion B/NGC 2024
- Evolutionary Status of Brightest and Youngest Source in the Orion Molecular Cloud-3 Region
- High angular resolution near-IR view of the Orion Bar revealed by Keck/NIRC2
- VLBA determination of the distance to nearby star-forming regions VII. Monoceros R2
- Depletion of chlorine into HCl ice in a protostellar core
- Expanding CO Shells in the Orion A Molecular Cloud
- Predicted Colors and Flux Densities of Protostars in the Herschel PACS and SPIRE Filters
- High Resolution Radio Astronomy Using Very Long Baseline Interferometry
- HST survey of the Orion Nebula Cluster in the HO 1.4 m absorption band: I. A census of substellar and planetary mass objects
- A New Halpha Emission-Line Survey in the Orion Nebula Cluster
- A High Spatial Resolution Study of the λ=3 mm Continuum of Orion-KL
- Probing the structure of a massive filament: ArTeMiS 350 and 450 micron mapping of the integral-shaped filament in Orion A
- AMI radio continuum observations of young stellar objects with known outflows
- Testing the models of X-ray driven photoevaporation with accreting stars in the Orion Nebula Cluster
- The water line emission and ortho-to-para ratio in the Orion Bar photon-dominated region
- The intrinsic abundance ratio and X-factor of CO isotopologues in L1551 shielded from FUV photodissociation
- ALMA Observations of the Largest Proto-Planetary Disk in the Orion Nebula, 114-426: A CO Silhouette
- [CII] line emission from Orion A. I. A template for extragalactic studies?
- Massive Protoplanetary Disks in Orion Beyond the Trapezium Cluster
- An Adaptive Optics Survey for Close Protostellar Binaries
- A global view on star formation: The GLOSTAR Galactic plane survey IV. Radio continuum detections of young stellar objects in the Galactic Centre region
- Quantitative inference of the column densities from 3 mm molecular emission: A case study towards Orion B
- Proper motions of molecular hydrogen outflows in the Rho Ophiuchi molecular cloud
- Extended ammonia observations towards the 'Integral-Shaped Filament'
- Herschel CHESS discovery of the fossil cloud that gave birth to the Trapezium and Orion KL
- A 3D View of Orion: I. Barnard's Loop
- Analysis of the Herschel/HEXOS Spectral Survey Towards Orion South: A massive protostellar envelope with strong external irradiation
- No evidence for intense, cold accretion onto YSOs from measurements of Li in T-Tauri stars
- Spatially Resolving Substructures within the Massive Envelope around an Intermediate-mass Protostar: MMS 6/OMC-3
- Orion revisited III. The Orion Belt population
- Searches for Interstellar HCCSH and HCCS
- CO Spectral Line Energy Distributions in Galactic Sources: Empirical Interpretation of Extragalactic Observations
- VISION - Vienna Survey in Orion II. Infrared extinction in Orion A
- The jet/counterjet IR symmetry of HH34 and the size of the jet formation region
- High Velocity Outflow in CO J=7-6 from the Orion Hot Core
- A VLBA Survey of radio stars in the Orion Nebula Cluster: I. The nonthermal radio population
- The Explosion in Orion-KL as Seen by Mosaicking the Magnetic Field with ALMA
- The Ionized Circumstellar Envelopes of Orion Source I and the Becklin Neugebauer Object
- Physical and chemical differentiation of the luminous star-forming region W49A - Results from the JCMT Spectral Legacy Survey
- PDRs4All XI. Detection of infrared CH and CH rovibrational emission in the Orion Bar and disk d203-506: evidence of chemical pumping
- Distribution of HNCO 5 in Massive Star-forming Regions
- The X-ray luminosity function of M37 and the evolution of coronal activity in low-mass stars
- The Origin of Ionized Filaments Within the Orion-Eridanus Superbubble
- Evidence for early disk-locking among low-mass members of the Orion Nebula Cluster
- Three-dimensional dust mapping in the Orion Complex, combining Gaia-TGAS, 2MASS, and WISE
- Optical interferometric observations of Theta 1 Orionis C from NPOI and implications for the system orbit
- Searching for Jet Rotation in Class 0/I Sources observed with GEMINI/GNIRS
- CARMA-NRO Orion Survey: unbiased survey of dense cores and core mass functions in Orion A
- First-generation Science Cases for Ground-based Terahertz Telescopes
- Polycyclic Aromatic Hydrocarbon emission model in photodissociation regions I: Application to the 3.3, 6.2, and 11.2 m bands
- The Stellar Content of Obscured Galactic Giant HII Regions. VII. W3
- HST astrometry in the Orion Nebula Cluster: census of low-mass runaways
- Origin of hydrogen fluoride emission in the Orion Bar: An excellent tracer for CO-dark H2 gas clouds
- The Structure of the Young Star Cluster NGC 6231. I. Stellar Population
- Mid-J CO emission from the Orion BN/KL explosive outflow
- The Orion fingers: Near-IR spectral imaging of an explosive outflow
- Disk and outflow signatures in Orion-KL: The power of high-resolution thermal infrared spectroscopy
- Layers in the Central Orion Nebula
- Breaking Orion's Veil bubble with fossil outflows
- Adaptive Optics Observations of 3 micron Water Ice in Silhouette Disks in the Orion Nebula Cluster and M43
- Probing the multi-scale interplay between gravity and turbulence - Power-law like gravitational energy spectra of the Orion Complex
- A Q-band line survey towards Orion KL using the Tianma radio telescope
- Observation and calibration strategies for large-scale multi-beam velocity-resolved mapping of the [CII] emission in the Orion molecular cloud
- Characterising the high-mass star forming filament G351.776--0.527 with Herschel and APEX dust continuum and gas observations
- Protostars at Low Extinction in Orion A
- Gas absorption and dust extinction towards the Orion Nebula Cluster
- Halpha emission-line stars in molecular clouds. II. The M42 region
- A Very Long Baseline Interferometry Detection of the Class I Protostar IRS 5 in Corona Australis
- Kompaneets Model Fitting of the Orion-Eridanus Superbubble
- A candidate planetary-mass object with a photoevaporating disk in Orion
- A VLBA Survey of radio stars in the Orion Nebula Cluster: II. Astrometry
- Orion Bar as a window to the evolution of PAHs
- High Resolution H alpha Images of the Binary Low-mass Proplyd LV 1 with the Magellan AO System
- The First Circumstellar Disk Imaged in Silhouette with Adaptive Optics: MagAO Imaging of Orion 218-354
- A Chemical Map of the Outbursting V883 Ori system: Vertical and Radial Structures
- The APEX Large CO Heterodyne Orion Legacy Survey (ALCOHOLS). I. Survey overview
- A large catalogue of molecular clouds in the southern sky
- Circumbinary disc survival during binary-single scattering: towards a dynamical model of the Orion BN/KL complex
- Multi-Scale Analysis of Magnetic Fields in Filamentary Molecular Clouds in Orion A
- Emergence of high-mass stars in complex fiber networks (EMERGE). I. Early ALMA Survey: observations and massive data reduction
- Parsec-scale cosmic-ray ionisation rate in Orion
- Empirical Near Infrared colors for low-mass stars and brown dwarfs in the Orion Nebula Cluster
- Herschel/HIFI observations of a new interstellar water maser: the 5(32)-4(41) transition at 620.701 GHz
- Characterizing the stellar population of NGC 1980
- Water and Methanol Maser Survey of Protostars in the Orion Molecular Cloud Complex
- On the Formation of Runaway Stars BN and x in the Orion Nebula Cluster
- Observations of Orion Source I Disk and Outflow Interface
- High Angular Resolution Observations at 7-mm of the Core of the Quadrupolar HH 111/121 Outflow
- Stellar and circumstellar properties of visual binaries in the Orion Nebula Cluster
- Gas kinematics around filamentary structures in the Orion B cloud
- Evidence for dense gas heated by the explosion in Orion KL
- Star Cluster Formation in Orion A
- HOPS 136: An Edge-On Orion Protostar Near the End of Envelope Infall
- ALMA Observation of the 658 GHz Vibrationally Excited HO Maser in Orion KL Source I
- Molecular tracers of radiative feedback in Orion (OMC-1). Widespread CH+ (J=1-0), CO (10-9), HCN (6-5), and HCO+ (6-5) emission
- SIRIUS Project. IV. The formation history of the Orion Nebula Cluster driven by clump mergers
- Magnetic Field Structure of Orion Source I
- Merged H/H2 and C+/C/CO transitions in the Orion Bar
- APEX-SEPIA660 Early Science: Gas at densities above cm towards OMC-1
- Hunting for the elusive methylene radical
- Physical Conditions and Kinematics of the Filamentary Structure in Orion Molecular Cloud 1
- Dents in the Veil: Protostellar feedback in Orion
- Integral field spectroscopy of M1-67. A Wolf-Rayet nebula with LBVN appearance
- The HH34 outflow as seen in [FeII]1.64um by LBT-LUCI
- 13CO and C18O J=2-1 mapping of the environment of the Class 0 protostellar core SMM 3 in Orion B9
- ALMA band 8 continuum emission from Orion Source I
- Three-dimensional Shock Structure of Orion KL Outflow with IGRINS
- Outflow-Confined HII regions. II. The Early Break-Out Phase
- The Role of Magnetic Fields in the Stability and Fragmentation of Filamentary Molecular Clouds: Two Case Studies at OMC-3 and OMC-4
- An APEX survey of outflow and infall toward the youngest protostars in Orion
- Nobeyama 45-m Mapping Observations toward Orion A. III. Multi-Line Observations toward an Outflow-shocked Region, OMC-2 FIR
- The sub-mm J=6-5 line of 13CO in Orion
- Exploring the effects of high-velocity flows in abundance determinations in H II regions. Bidimensional spectroscopy of HH 204 in the Orion Nebula
- Evidence for a Photoevaporated Circumbinary Disk in Orion
- Kinematics of the Orion Trapezium Based on Diffracto-Astrometry and Historical Data
- Nano-grain depletion in photon-dominated regions
- Magnetic Field of Molecular Gas Measured with the Velocity Gradient Technique I. Orion A
- Structure of the Source I disk in Orion-KL
- The Cygnus Allscale Survey of Chemistry and Dynamical Environments: CASCADE. II. A detailed kinematic analysis of the DR21 Main outflow
- Exploring morphological correlations among H2CO, 12CO, MSX and continuum mappings
- NH (1,1) hyperfine intensity anomalies in the Orion A molecular cloud
- The Column Density Structure of Orion A Depicted by N-PDF
- A spectroscopic survey of Orion KL between 41.5 and 50 GHz
- The Orion fingers: H temperatures and excitation in an explosive outflow
- X-ray deficiency on strong accreting T Tauri stars - Comparing Orion with Taurus
- The Radio-X-ray Connection in Young Stellar Objects in the Orion Nebula Cluster
- Large-scale CO (J=4-3) Mapping toward the Orion-A Giant Molecular Cloud
- Emergence of high-mass stars in complex fiber networks (EMERGE) II. The need for data combination in ALMA observations
- Young Stellar Object candidates toward the Orion region selected from GALEX
- Infall and rotation motions in the HH 111 protostellar system: A flattened envelope in transition to a disk?
- The GBT 67 -- 93.6 GHz Spectral Line Survey of Orion-KL
- A kinematic analysis of the CO clouds toward a reflection nebula NGC 2023 observed with the Nobeyama 45 m telescope; Further evidence for a cloud-cloud collision in the Orion region
- APEX Observations of the CO Envelope around the Young FUor-type Star V883 Ori
- The richness of compact radio sources in NGC 6334D to F
- Keck Adaptive Optics Observations of the Protostellar Disk around Radio Source I in the Orion Kleinmann-Low Nebula
- High Cadence Time-Series Photometry of V1647 Orionis
- The ionization fraction in OMC-2 and OMC-3
- An imaging line survey of OMC-1 to OMC-3
- First Resolved Dust Continuum Measurements of Individual Giant Molecular Clouds in the Andromeda Galaxy
- Relative alignment between gas structures and magnetic field in Orion A at different scales using different molecular gas tracers
- Resolving the Binary Components of the Outbursting Protostar HBC 494 with ALMA
- The CARMA-NRO Orion Survey: Statistical Signatures of Feedback in the Orion A Molecular Cloud
- Multiline observations of hydrogen, helium, and carbon radio-recombination lines toward Orion A: A detailed dynamical study and direct determination of physical conditions
- Extremely high excitation SiO lines in disk-outflow system in Orion Source I
- Orbital Solution for the Spectroscopic Binary in the GW Ori Hierarchical Triple
- Massive Quiescent Cores in Orion: VI. The Internal Structures and a Candidate of Transiting Core in NGC 2024 Filament
- The CO core mass function toward Orion A: Single-dish observations
- Using deuterated H3+ and other molecular species to understand the formation of stars and planets
- Externally irradiated young stars in NGC 3603. A JWST NIRSpec catalogue of pre-main-sequence stars in a massive star formation region
- The structure and kinematics of dense gas in NGC 2068
- A Molecular Line Survey around Orion at Low Frequencies with the MWA
- Mid- CO Line Observations of Protostellar Outflows in the Orion Molecular Clouds
- ALMA Observations of Asymmetric Molecular Gas Emission from a Protoplanetary Disk in the Orion Nebula
- The Structure of NGC 1976 in the Radio Range
- The System of Molecular Clouds in the Gould Belt
- Massive Quiescent Cores in Orion: V. The Physical Structures on Sub-Jeans Scale and the Chemical Properties in Two Extremely Dense Cores
- Near infrared view on the photodissociation regions S255, S257, NGC7538 and S140
- High spectral resolution observations toward Orion BN at 6 m: no evidence for hot water
- The evolution of the X-ray emission of HH 2 - Investigating heating and cooling processes
- ALMA view of the Ophiuchi A PDR with a 360-au beam: the [CI] emission originates from the plane-parallel PDR and extended gas
- Residual HCRF Rotation relative to the Inertial Coordinate System
- SABOCA 350-micron and LABOCA 870-micron dust continuum imaging of IRAS 05399-0121: mapping the dust properties of a pre- and protostellar core system
- Emergence of high-mass stars in complex fiber networks (EMERGE) III. Fiber networks in Orion
- CARMA = 1 cm Spectral Line Survey of Orion-KL
- XMM-Newton imaging of V1818 Ori: a young stellar group on the eastern edge of the Kappa Ori ring
- Symmetry properties and widths of the filamentary structures in the Orion A giant molecular cloud
- Emergence of high-mass stars in complex fiber networks (EMERGE) IV. Environmental dependence of the fiber widths
- A contracting circumbinary molecular ring with an inner cavity of about 140 AU around Ori 139-409
- An ionized outflow in Orion-KL source I?
- The distribution of deuterated formaldehyde within Orion-KL
- Modelling the CO streamers in the explosive ejection of Orion BN/KL region
- Dynamical masses of YSOs with the VLBA: DYNAMO VLBA: Trigonometric parallaxes and proper motions of YSOs in Orion
- History of Globulettes in the Milky Way
- Continuum, CO and Water vapour maps of the Orion Nebula. First millimetre spectral imaging with Concerto
- A CO observation of the galactic methanol masers
- The time evolution of HH~2 from four epochs of HST images
- Using Molecular Gas Observations to Guide Initial Conditions for Star Cluster Simulations
- Tracing PAH Size in Prominent Nearby Mid-Infrared Environments
- Detection of Dust Condensations in the Orion Bar Photon-dominated Region
- Accretion in low-mass members of the Orion Nebula Cluster with young transition disks
- Échelle Spectroscopy of the Chemically Peculiar Star Ori F
- A low-mass hub-filament with double centre revealed in NGC2071-North
- Molecular complexity on disk-scales uncovered by ALMA: The chemical composition of the high-mass protostar AFGL 4176
- COBRaS: The e-MERLIN 21 cm Legacy survey of Cygnus OB2
- The Effelsberg survey of FU~Orionis and EX~Lupi objects II. -- HO maser observations
- C2H, HC3N and HNC Observations in OMC-2/3
- PDRs4All XVII: Formation and excitation of HD in photodissociation regions. Application to the Orion Bar
- Beetroots: spatially-regularized Bayesian inference of physical parameter maps -- Application to Orion
- Spectropolarimetry of Magnetic Chemically Peculiar Stars in the Orion OB1 Association
- Characterizing the PAH Emission in the Orion Bar
- The Kinematic and Dynamic Properties of HBC 494's Wide-Angle Outflows
- On the Evolution of BM Orionis
- Photoevaporation of protoplanetary disks by Far-UV photons arising from neighbouring massive stars: observation of proplyds and modelling
- Scattered light signatures of flyby-induced warps in protoplanetary discs
- The Neutral Atomic Hydrogen in the solar neighborhood (NeAtHood) project I. Ghost in the shell: Neutral atomic hydrogen in the extended Orion nebula
- Linking Young Stellar Object Morphology to Evolutionary Stages with Self-Organizing Maps