Improved Measurements of Molecular Cloud Distances Based on Global Search
arXiv:2108.11046 · doi:10.3847/1538-4357/ac214f
Abstract
The principle of the background-eliminated extinction-parallax (BEEP) method is examining the extinction difference between on- and off-cloud regions to reveal the extinction jump caused by molecular clouds, thereby revealing the distance in complex dust environments. The BEEP method requires high-quality images of molecular clouds and high-precision stellar parallaxes and extinction data, which can be provided by the Milky Way Imaging Scroll Painting (MWISP) CO survey and the Gaia DR2 catalog, as well as supplementary AV extinction data. In this work, the BEEP method is further improved (BEEP-II) to measure molecular cloud distances in a global search manner. Applying the BEEP-II method to three regions mapped by the MWISP CO survey, we collectively measured 238 distances for 234 molecular clouds. Compared with previous BEEP results, the BEEP-II method measures distances efficiently, particularly for those molecular clouds with large angular size or in complicated environments, making it suitable for distance measurements of molecular clouds in large samples.
Accepted for publication in ApJ. 17 pages, 8 figures
References in corpus (19)
- The Gaia mission
- Trigonometric Parallaxes of Massive Star Forming Regions: VI. Galactic Structure, Fundamental Parameters and Non-Circular Motions
- Trigonometric Parallaxes Of High-Mass Star Forming Regions: Our View Of The Milky Way
- Structural Analysis of Molecular Clouds: Dendrograms
- Physical properties of molecular clouds for the entire Milky Way disk
- A Large Catalog of Accurate Distances to Local Molecular Clouds: The Gaia DR2 Edition
- A Compendium of Distances to Molecular Clouds in the Star Formation Handbook
- The Milky Way Imaging Scroll Painting (MWISP): Project Details and Initial Results from the Galactic Longitude of 25.8deg to 49.7deg
- The SEDIGISM survey: first data release and overview of the Galactic structure
- Identification of Young Stellar Object candidates in the DR2 x AllWISE catalogue with machine learning methods
- The integrated properties of the molecular clouds from the JCMT CO(3-2) High Resolution Survey
- The SEDIGISM survey: Molecular clouds in the inner Galaxy
- The Distances to Molecular Clouds at High Galactic Latitudes based on GAIA DR2
- A 3D view of the Taurus star-forming region by Gaia and Herschel: multiple populations related to the filamentary molecular cloud
- Distances and statistics of local molecular clouds in the first Galactic quadrant
- Molecular gas distribution perpendicular to the Galactic plane
- Distances to molecular clouds in the second Galactic quadrant
- Local Molecular Gas toward the Aquila Rift Region
- On the Beam Filling Factors of Molecular Clouds
Cited by in corpus (6)
- Distances to nearby molecular clouds traced by young stars
- Dependence of Molecular Cloud Samples on Angular Resolution, Sensitivity, and Algorithms
- On the Spatial Distribution of CO Structures within CO Molecular Clouds
- New method for estimating molecular cloud distances based on Gaia, 2MASS, and the TRILEGAL galaxy model
- Examining Turbulence in Galactic Molecular Clouds -- I: A Statistical Analysis of Velocity Structures
- Distance estimation of the high-velocity cloud Anti-Center Shell