J/ApJS/280/16  All-sky cat. of molecular clouds from 3D dust map  (Wang+, 2025)

A comprehensive all-sky catalog of 3345 molecular clouds from three-dimensional dust extinction. Wang T., Yuan H., Chen B., Li G., Huang B., Guo H., Zhang R. <Astrophys. J. Suppl. Ser., 280, 16 (2025)> =2025ApJS..280...16W 2025ApJS..280...16W
ADC_Keywords: Molecular clouds; Interstellar medium; Milky Way; Optical; Extinction Keywords: Interstellar dust ; Interstellar medium ; Milky Way Galaxy ; Molecular clouds ; Catalogs Abstract: Understanding the distribution and properties of molecular clouds is crucial for tracing the structure and evolution of the interstellar medium (ISM) and the large-scale morphology of the Milky Way. Here we present an all-sky catalog of 3345 molecular clouds identified from our previous three-dimensional dust-reddening map using a dendrogram-based clustering method with distance-adaptive parameters. The catalog spans heliocentric distances from 90pc to 4.3kpc and includes key physical properties for each cloud, including position, size, mass, surface density, and dust density. Approximately 650 clouds in our catalog are associated with the boundary of the Local Bubble, while around 740 clouds (excluding those associated with the Local Bubble) are located at high Galactic latitudes (|b|>20). The spatial distribution of the cataloged clouds reveals prominent large-scale features in the Galactic disk, including coherent spur-like structures, large-scale cavities, and a more detailed view of the Local Bubble shell. These findings refine our understanding of how molecular clouds trace the Galactic spiral arm network and provide new insight into the spatial structure of the Local Bubble. The catalog serves as a valuable resource for future studies of star formation, Galactic structure, and the interaction between molecular clouds and large-scale ISM features. Description: This study uses the 3D dust-reddening map published by W25 (Wang+ 2025, J/ApJS/280/15), which provides an all-sky view of the reddening distribution. The map was constructed by combining reddening measurements from two major sources: low-resolution spectra from the Large Sky Area Multi-Object Fiber Spectroscopy Telescope (LAMOST) DR11 and BP/RP (hereafter XP) spectra from the European Space Agency's Gaia mission. The 3D dust map used in this study is publicly available from the website https://nadc.china-vo.org/data/dustmaps File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file table2.dat 57 3345 Catalog of molecular clouds -------------------------------------------------------------------------------- See also: I/337 : Gaia DR1 (Gaia Collaboration, 2016) I/355 : Gaia DR3 Part 1. Main source (Gaia Collaboration, 2022) J/A+A/327/325 : Distances of molecular cloud (May+, 1997) J/A+A/411/447 : Interstellar NaI D-line (Lallement+, 2003) J/A+A/591/A5 : ATLASGAL dense filamentary structures (Li+, 2016) J/ApJ/834/57 : MW molecular clouds from 12CO (Miville-Deschenes+, 2017) J/MNRAS/487/1400 : Spiral structure as revealed by O and B stars (Chen+, 2019) J/ApJ/885/131 : High-mass SFR plx & proper motion with VLBI (Reid+, 2019) J/MNRAS/493/351 : A large catalogue of molecular clouds (Chen+, 2020) J/MNRAS/511/2302 : Molecular clouds study from 3D extinction maps (Guo+, 2022) J/A+A/664/A174 : Gal. interstellar dust Gaia-2MASS 3D maps (Vergely+, 2022) J/AJ/168/203 : Dust clouds masses, color excesses & distances (Sun+, 2024) J/ApJS/280/15 : Extinction catalog from Gaia DR3 & LAMOST DR11 (Wang+, 2025) Byte-by-byte Description of file: table2.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 4 I4 --- Seq [1/3345] Sequential identifier 6- 11 F6.2 deg GLON Galactic longitude 13- 18 F6.2 deg GLAT [-87.12/87.2] Galactic latitude 20- 23 F4.2 kpc Dist [0.09/4.3] Distance 25- 30 F6.2 pc Rad [1.65/148.11] Projected radius 32- 36 F5.2 deg2 Area [0.2/86.58] Angular area 38- 43 E6.2 Msun Mass [4.11/629000.0] Total mass 45- 49 F5.2 Msun.pc-2 Sigma [0.28/41.98] Surface density 51- 55 F5.2 mag.kpc-1 rho [0.09/11.99] Average dust column density 57- 57 I1 --- Flag [0/1] Local Bubble Flag (1) -------------------------------------------------------------------------------- Note (1): The Local Bubble flag indicates whether the cloud is located on the boundary of the Local Bubble (1 = yes, 0 = no). -------------------------------------------------------------------------------- History: From electronic version of the journal
(End) Prepared by [AAS], Emmanuelle Perret [CDS] 25-Mar-2026
The document above follows the rules of the Standard Description for Astronomical Catalogues; from this documentation it is possible to generate f77 program to load files into arrays or line by line