The spiral structure in the Solar neighborhood
arXiv:2110.04446 · doi:10.3389/fspas.2021.671670
Abstract
The spiral structure in the Solar neighborhood is an important issue in astronomy. In the past few years, there is significant progress in observation. The distances for a large number of good spiral tracers, i.e. giant molecular clouds, high-mass star-formation region masers, HII regions, O-type stars and young open clusters, have been accurately estimated, making it possible to depict the detailed properties of nearby spiral arms. In this work, we first give an overview about the research status for the Galaxy's spiral structure based on different types of tracers. Then the objects with distance uncertainties better than 15\% and 0.5 kpc are collected and combined together to depict the spiral structure in the Solar neighborhood. Five segments related with the Perseus, Local, Sagittarius-Carina, Scutum-Centaurus and Norma Arms are traced. With the large dataset, the parameters of the nearby arm segments are fitted and updated. Besides the dominant spiral arms, some substructures probably related to arm spurs or feathers are also noticed and discussed.
arXiv comment23 pages, 4 figures, published in Frontiers in Astronomy and Space Sciences as a REVIEW article
References in corpus (112)
- Gaia Data Release 2. Summary of the contents and survey properties
- The Gaia mission
- The Milky Way in Molecular Clouds: A New Complete CO Survey
- A Hipparcos census of the nearby OB associations
- A New Electron Density Model for Estimation of Pulsar and FRB Distances
- Trigonometric Parallaxes of Massive Star Forming Regions: VI. Galactic Structure, Fundamental Parameters and Non-Circular Motions
- New catalogue of optically visible open clusters and candidates
- Trigonometric Parallaxes Of High-Mass Star Forming Regions: Our View Of The Milky Way
- Global survey of star clusters in the Milky Way II. The catalogue of basic parameters
- A Gaia DR2 view of the Open Cluster population in the Milky Way
- Galaxy Zoo 2: detailed morphological classifications for 304,122 galaxies from the Sloan Digital Sky Survey
- Painting a portrait of the Galactic disc with its stellar clusters
- Three Dimensional Structure of the Milky Way Disk
- The WISE Catalog of Galactic HII Regions
- Physical properties of molecular clouds for the entire Milky Way disk
- Star Formation Efficiencies and Lifetimes of Giant Molecular Clouds in the Milky Way
- The Distance to the Perseus Spiral Arm in the Milky Way
- The Structure of the Milky Way's Bar Outside the Bulge
- Updated parameters of 1743 open clusters based on Gaia DR2
- Clusters and mirages: cataloguing stellar aggregates in the Milky Way
- The observed spiral structure of the Milky Way
- The wobbly Galaxy: kinematics north and south with RAVE red clump giants
- Dawes Review 4: Spiral Structures in Disc Galaxies
- Age determination for 269 DR2 Open Clusters
- Self-Perpetuating Spiral Arms in Disk Galaxies
- Gas Dynamics in the Milky Way: Second Pattern Speed and Large-Scale Morphology
- Untangling the Galaxy I: Local Structure and Star Formation History of the Milky Way
- The Spiral Structure of the Outer Milky Way in Hydrogen
- Hunting for open clusters in \textit{Gaia} DR2: new OCs in the Galactic disc
- ON the Nature of the Local Spiral Arm of the Milky Way
- A new method for unveiling Open Clusters in Gaia: new nearby Open Clusters confirmed by DR2
- A Uniform Catalog of Molecular Clouds in the Milky Way
- Fundamental Parameters of the Milky Way Galaxy Based on VLBI astrometry
- Three-dimensional interstellar dust reddening maps of the Galactic plane
- Gas flow models in the Milky Way embedded bars
- The RMS Survey: Galactic distribution of massive star formation
- Direct determination of the spiral pattern rotation speed of the Galaxy
- Trigonometric Parallaxes of 6.7 GHz Methanol Masers
- The spiral structure of our Milky Way Galaxy
- 3D kinematics and age distribution of the Open Cluster population
- Hunting for open clusters in \textit{Gaia} DR2: the Galactic anticentre
- Three-Dimensional Distribution of the ISM in the Milky Way Galaxy: III. The Total Neutral Gas Disk
- Radial and vertical flows induced by galactic spiral arms: likely contributors to our "wobbly Galaxy''
- The structure of spiral galaxies - II. Near-infrared properties of spiral arms
- Improving the open cluster census. I. Comparison of clustering algorithms applied to Gaia DR2 data
- Radial Distribution of Stellar Motions in Gaia DR2
- Spatial distribution of Galactic HII regions
- Gaia DR2 unravels incompleteness of nearby cluster population: New open clusters in the direction of Perseus
- Spurs and feathering in spiral galaxies
- Resonance sweeping by a decelerating Galactic bar
- Characteristics of the Galaxy according to Cepheids
- 3D Distribution of Molecular Gas in the Barred Milky Way
- The signatures of the resonances of a large Galactic bar in local velocity space
- Spiral structure in the outer Galactic disk. I. The Third Galactic Quadrant
- Spiral structure of the Third Galactic Quadrant and the solution to the Canis Major debate
- The First VERA Astrometry Catalog
- OB associations and their origins
- The local spiral structure of the Milky Way
- An HST Archival Survey of Feathers in Spiral Galaxies
- Signatures of resonance and phase mixing in the Galactic disc
- Age distributions of star clusters in spiral and barred galaxies as a test for theories of spiral structure
- Finding Distant Galactic HII Regions
- Spiral structure in nearby galaxies I. Sample, data analysis, and overview of results
- A comparison of the local spiral structure from Gaia DR2 and VLBI maser parallaxes
- Spectrophotometric Distances to Galactic H\,{\sc{ii}} Regions
- The spiral pattern rotation speed of the Galaxy and the corotation radius with GAIA DR2
- A Multi-Membership Catalogue for 1876 Open Clusters using UCAC4 data
- Giant molecular clouds and massive star formation in the southern milky way
- The Milky Way Spiral Structure Parameters from Data on Masers and Selected Open Clusters
- The Catalogue of Stellar Parameters from the Detached Double-Lined Eclipsing Binaries in the Milky Way
- Identifying resonances of the Galactic bar in Gaia DR2: I. Clues from action space
- Offset between stellar spiral arms and gas arms of the Milky Way
- The Alma catalog of OB stars. II. A cross-match with Gaia DR2 and an updated map of the solar neighbourhood
- A large catalogue of molecular clouds with accurate distances within 4 kpc of the Galactic disk
- Branch, Spur, and Feather Formation in Spiral Galaxies
- The morphology of the Milky Way - I. Reconstructing CO maps from simulations in fixed potentials
- The SEDIGISM survey: Molecular clouds in the inner Galaxy
- Evolution of the local spiral structure of the Milky Way revealed by open clusters
- The shapes of spiral arms in the SG survey and their connection with stellar bars
- The spiral structure of the Milky Way
- Hic sunt dracones: Cartography of the Milky Way spiral arms and bar resonances with Gaia Data Release 2
- Detection of a young stellar population in the background of open clusters in the Third Galactic Quadrant
- The Galactic spiral structure as revealed by O- and early B-type stars
- Local spiral structure based on the Gaia EDR3 parallaxes
- The Bar and Spiral Arms in the Milky Way: Structure and Kinematics
- A CGPS Look at the Spiral Structure of the Outer Milky Way I: Distances and Velocities to Star Forming Regions
- Discovery and astrophysical properties of Galactic open clusters in dense stellar fields using Gaia DR2
- On the Interpretation of the l-v Features in the Milky Way Galaxy
- A catalogue of 74 new open clusters found in Gaia Data-Release 2
- The morphology of the Milky Way - II. Reconstructing CO maps from disc galaxies with live stellar distributions
- Global survey of star clusters in the Milky Way IV. 63 new open clusters detected by proper motions
- Characteristics of Spiral Arms in Late-type Galaxies
- The Carnegie-Irvine Galaxy Survey. VI. Quantifying Spiral Structure
- Tracing the Spiral Structure of the Outer Milky Way with Dense Atomic Hydrogen Gas
- Distances and statistics of local molecular clouds in the first Galactic quadrant
- New star clusters discovered towards the Galactic bulge direction using Gaia DR2
- The spiral structure of the Galaxy revealed by CS sources and evidence for the 4:1 resonance
- The dynamical origin of the Local arm and the Sun's trapped orbit
- Parallaxes of 6.7-GHz Methanol Masers towards the G305.2 High-Mass Star Formation Region
- Molecular cloud distances based on the MWISP CO survey and Gaia DR2
- FEDReD II : 3D Extinction Map with 2MASS and Gaia DR2 data
- First detection of the field star overdensity in the Perseus arm
- Combined dynamical effects of the bar and spiral arms in a Galaxy model. Application to the solar neighbourhood
- Distances to molecular clouds in the second Galactic quadrant
- A search of the Orion spur for continuous gravitational waves using a "loosely coherent" algorithm on data from LIGO interferometers
- Stellar Overdensity in the Local Arm in Gaia DR2
- The power of co-ordinate transformations in dynamical interpretations of Galactic structure
- Towards a census of the Galactic anticentre star clusters - III: tracing the spiral structure in the Outer Disk
- Update of membership and mean proper motion of open clusters from UCAC5 catalog
- First results from a large-scale proper motion study of the Galactic Centre
- The local spiral arm in the LAMOST-Gaia common stars?
- Offsets of masers with respect to the middle of the Perseus arm, and the co-rotation radius in the Milky Way
Cited by in corpus (19)
- Gaia Data Release 3: Mapping the asymmetric disc of the Milky Way
- New Open Cluster candidates Found in Galactic Disk Using Gaia DR2/EDR3 Data
- What Does the Milky Way Look Like?
- Tracing the Milky Way warp and spiral arms with classical Cepheids
- Westerlund 1 under the light of Gaia EDR3: Distance, isolation, extent, and a hidden population
- An investigation of open clusters Berkeley 68 and Stock 20 using CCD UBV and Gaia DR3 data
- Large-scale Velocity-coherent Filaments in the SEDIGISM Survey: Association with Spiral Arms and Fraction of Dense Gas
- Peering into the Milky Way by FAST: IV. Identification of two new Galactic supernova remnants G203.1+6.6 and G206.7+5.9
- Catalog of spiral arm Tangents (Galactic Longitudes) in the Milky Way, and the Age Gradient based on various arm tangents
- Parallax-based Distances to Galactic Hii Regions: Nearby Spiral Structure
- The Outer spiral arm of the Milky Way using Red Clump stars
- On the nature of rotation in the Praesepe cluster
- Redetermination of the Parameters of the Galactic Spiral Pattern from Classical Cepheids
- Topography of the Young Galactic Disk: Spatial and Kinematic Patterns of the Clustered Star Formation in the Solar Neighborhood
- Estimation of the Parameters of the Spiral Pattern in the Galaxy Based on a Sample of Classical Cepheids
- A cosmic-ray loaded nascent outflow driven by a massive star cluster
- The Galactic inner spiral arms revealed by the Gaia ESO Survey chemical abundances. Metallicity and [Mg/Fe] ratios
- Galaxy rotation curve based on RGB stars from the Gaia DR3 catalogue
- The MAGIC project. III. Radial and azimuthal Galactic abundance gradients using classical Cepheids