[WTG2015] G47 , the SIMBAD biblio

[WTG2015] G47 , the SIMBAD biblio (12 results) C.D.S. - SIMBAD4 rel 1.8 - 2024.02.22CET22:14:28

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Bibcode/DOI Score in Title|Abstract|
in a table in teXt, Caption, ... Nb occurence Nb objects in ref Citations
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Title First 3 Authors
2015MNRAS.450.4043W 177       D       C F     3 24 118 Large-scale filaments associated with Milky Way spiral arms. WANG K., TESTI L., GINSBURG A., et al.
2015ApJ...815...23Z 41           X         1 30 68 The skeleton of the Milky Way. ZUCKER C., BATTERSBY C. and GOODMAN A.
2016A&A...591A...5L viz 18       D               1 42 87 ATLASGAL: A Galaxy-wide sample of dense filamentary structures. LI G.-X., URQUHART J.S., LEURINI S., et al.
2016ApJS..226....9W 40           X         1 78 60 A census of large-scale (>=10 PC), velocity-coherent, dense filaments in the northern galactic plane: automated identification using minimum spanning tree. WANG K., TESTI L., BURKERT A., et al.
2018A&A...609A..43X 3029 T K A S   X C       71 17 4 Gas kinematics and star formation in the filamentary molecular cloud
XU J.-L., XU Y., ZHANG C.-P., et al.
2018ApJ...864...54D 41           X         1 17 1 Filamentary structures and star formation activity in the sites S234, V582, and IRAS 05231+3512. DEWANGAN L.K., BAUG T., OJHA D.K., et al.
2019A&A...622A..52Z 685       D     X C       16 81 42 Star-forming content of the giant molecular filaments in the Milky Way. ZHANG M., KAINULAINEN J., MATTERN M., et al.
2019A&A...627A..27X viz 84           X         2 14 ~ The effects of ionization feedback on star formation: a case study of the M 16 H II region. XU J.-L., ZAVAGNO A., YU N., et al.
2022ApJ...926L...6S 1326 T   A     X C       28 6 4 The Magnetic Field in the Milky Way Filamentary Bone
2023ApJ...953...66N 93           X         2 14 ~ B-fields and Dust in Interstellar Filaments Using Dust Polarization (BALLAD-POL). I. The Massive Filament G11.11-0.12 Observed by SOFIA/HAWC+. NGOC N.B., DIEP P.N., HOANG T., et al.
2024A&A...681A..51W 320       D     X C       6 32 ~ The role of turbulence in high-mass star formation: Subsonic and transonic turbulence are ubiquitously found at early stages. WANG C., WANG K., XU F.-W., et al.
2024ApJ...961..124Z 550     A D     X C       11 13 ~ Magnetic Fields in Giant Filaments Probed by the Velocity Gradient Technique: Regular Magnetic Field Interrupted by Magnetization Gaps. ZHAO M., LI G.-X., ZHOU J., et al.

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