The Gould's Belt Distances Survey (GOBELINS) II. Distances and structure towards the Orion Molecular Clouds
arXiv:1609.04041 · doi:10.3847/1538-4357/834/2/142
Abstract
We present the results of the Gould's Belt Distances Survey (GOBELINS) of young star forming regions towards the Orion Molecular Cloud Complex. We detected 36 YSOs with the Very Large Baseline Array (VLBA), 27 of which have been observed in at least 3 epochs over the course of 2 years. At least half of these YSOs belong to multiple systems. We obtained parallax and proper motions towards these stars to study the structure and kinematics of the Complex. We measured a distance of 3885 pc towards the Orion Nebula Cluster, 42810 pc towards the southern portion L1641, 38810 pc towards NGC 2068, and roughly 420 pc towards NGC 2024. Finally, we observed a strong degree of plasma radio scattering towards Ori.
arXiv commentAccepted for publication to ApJ
References in corpus (39)
- A Survey of Stellar Families: Multiplicity of Solar-Type Stars
- Stellar Multiplicity
- The distance to the Orion Nebula
- The Proper Motion of Sgr A*: II. The Mass of Sgr A*
- The Spitzer Space Telescope Survey of the Orion A & B Molecular Clouds - Part I: A Census of Dusty Young Stellar Objects and a Study of their Mid-IR Variability
- A Correlation Between Surface Densities of Young Stellar Objects and Gas in Eight Nearby Molecular Clouds
- A Large Catalog of Accurate Distances to Molecular Clouds from PS1 Photometry
- Micro-Arcsecond Radio Astrometry
- The Gould's Belt Distances Survey (GOBELINS) I. Trigonometric parallax distances and depth of the Ophiuchus complex
- Distance to Orion KL Measured with VERA
- A Multi-color Optical Survey of the Orion Nebula Cluster. II. the H-R diagram
- A Parallactic Distance of 389 +24/-21 parsecs to the Orion Nebula Cluster from Very Long Baseline Array Observations
- A VLBI Resolution of the Pleiades Distance Controversy
- Binary Stars in the Orion Nebula Cluster
- The Gould's Belt Distances Survey (GOBELINS) III. The distance to the Serpens/Aquila Molecular Complex
- Revealing the physical properties of molecular gas in Orion with a large scale survey in J=2-1 lines of 12CO, 13CO and C18O
- Tracing the young massive high-eccentricity binary system Theta 1 Orionis C through periastron passage
- IN-SYNC IV - The Young Stellar Population in the Orion A Molecular Cloud
- Dynamical Mass Constraints on Low-Mass Pre-Main-Sequence Stellar Evolutionary Tracks: An Eclipsing Binary in Orion with a 1.0 Msun Primary and an 0.7 Msun Secondary
- Monitoring the Large Proper Motions of Radio Sources in the Orion BN/KL Region
- Orion Revisited - I. The massive cluster in front of the Orion Nebula Cluster
- Diffraction-limited Visible Light Images of Orion Trapezium Cluster With the Magellan Adaptive Secondary AO System (MagAO)
- The Smallest Mass Ratio Young Star Spectroscopic Binaries
- A Multi-Epoch Study of the Radio Continuum Emission of Orion Source I: Constraints on the Disk Evolution of a Massive YSO and the Dynamical History of Orion BN/KL
- N-body simulations of stars escaping from the Orion nebula
- A Photometric Study of the Young Stellar Population Throughout the lambda Orionis Star-Forming Region
- Main-Seqence Fitting Distance to the sigma Ori Cluster
- The distance to the Orion Nebula Cluster
- Nested shells reveal the rejuvenation of the Orion-Eridanus superbubble
- Orion revisited. II. The foreground population to Orion A
- Evidence for Environmental Dependence of the Upper Stellar Initial Mass Function in Orion A
- 7 mm lambda VLBA Observations of Sagittarius A*
- YSOVAR: Six pre-main-sequence eclipsing binaries in the Orion Nebula Cluster
- The Gould's Belt Very Large Array Survey III. The Orion region
- Spectroscopic Binaries in the Orion Nebula Cluster and NGC 2264
- The multiplicity of massive stars in the Orion Nebula cluster as seen with long-baseline interferometry
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- The Magnetic Field of the H~II Region NGC 6334A
- HST Images Do Not Support the Presence of Three High Velocity, Low-Mass Stars in the Core of the Orion Nebula Cluster
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