SDC G14.225-0.506 , the SIMBAD biblio

SDC G14.225-0.506 , the SIMBAD biblio (22 results) C.D.S. - SIMBAD4 rel 1.8 - 2024.04.18CEST11:06:52


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Title First 3 Authors
2009A&A...505..405P viz 15       D               1 11300 257 The initial conditions of stellar protocluster formation. I. A catalogue of Spitzer dark clouds. PERETTO N. and FULLER G.A.
2013ApJ...764L..26B 689 T K A     X C       16 11 70 Unveiling a network of parallel filaments in the infrared dark cloud

G14.225-0.506
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BUSQUET G., ZHANG Q., PALAU A., et al.
2013ApJ...772...69G 39           X         1 33 56 DR 21(OH): a highly fragmented, magnetized, turbulent dense core. GIRART J.M., FRAU P., ZHANG Q., et al.
2014MNRAS.440.2860H 41           X         1 20 102 The dynamical properties of dense filaments in the infrared dark cloud G035.39-00.33. HENSHAW J.D., CASELLI P., FONTANI F., et al.
2014ApJ...789...37V 380     A     X C       9 8 34 Core and filament formation in magnetized, self-gravitating isothermal layers. VAN LOO S., KETO E. and ZHANG Q.
2014ApJ...797...76L 39           X         1 40 30 CARMA large area star formation survey: structure and kinematics of dense gas in Serpens main. LEE K.I., FERNANDEZ-LOPEZ M., STORM S., et al.
2015ApJ...811..134S 40           X         1 32 6 The dense filamentary giant molecular cloud G23.0-0.4: birthplace of ongoing massive star formation. SU Y., ZHANG S., SHAO X., et al.
2016A&A...590A..72P viz 16       D               1 11296 12 The initial conditions for stellar protocluster formation. III. The Herschel counterparts of the Spitzer Dark Cloud catalogue. PERETTO N., LENFESTEY C., FULLER G.A., 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.
2016ApJ...832..186S 1672 T K A     X C       40 10 20 Magnetically dominated parallel interstellar filaments in the infrared dark cloud

G14.225-0.506
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SANTOS F.P., BUSQUET G., FRANCO G.A.P., et al.
2017ApJ...836..199H viz 42           X         1 5 8 Tracing the magnetic field of IRDC G028.23-00.19 using NIR polarimetry. HOQ S., CLEMENS D.P., GUZMAN A.E., et al.
2017ApJ...840...22L 1384     A D     X C       34 9 31 Cloud structure of three galactic infrared dark star-forming regions from combining ground- and space-based bolometric observations. LIN Y., LIU H.B., DALE J.E., et al.
2018ApJS..234...28L 83           X         2 26 49 The TOP-SCOPE survey of Planck Galactic cold clumps: survey overview and results of an exemplar source, PGCC G26.53+0.17. LIU T., KIM K.-T., JUVELA M., et al.
2018A&A...610A..77H viz 44           X         1 45 159 An ALMA study of the Orion Integral Filament. I. Evidence for narrow fibers in a massive cloud. HACAR A., TAFALLA M., FORBRICH J., et al.
2019ApJ...873...31K 42           X         1 21 2 The core mass function in the infrared dark cloud G28.37+0.07. KONG S.
2019ApJ...876...42W 46           X         1 11 44 JCMT BISTRO survey: magnetic fields within the hub-filament structure in IC 5146. WANG J.-W., LAI S.-P., ESWARAIAH C., et al.
2020ApJ...903...13D 85           X         2 38 20 New insights into the H II region G18.88-0.49: hub-filament system and accreting filaments. DEWANGAN L.K., OJHA D.K., SHARMA S., et al.
2020ApJ...903...46C 198     A     X         5 4 10 Simultaneous evolution of the virial parameter and star formation rate in molecular clumps undergoing global hierarchical collapse. CAMACHO V., VAZQUEZ-SEMADENI E., PALAU A., et al.
2021MNRAS.504.1152D 44           X         1 14 7 Unraveling the inner substructure of new candidate hub-filament system in the H II region G25.4NW. DEWANGAN L.K.
2022ApJ...931..115W 45           X         1 19 4 Formation of the SDC13 Hub-filament System: A Cloud-Cloud Collision Imprinted on the Multiscale Magnetic Field. WANG J.-W., KOCH P.M., TANG Y.-W., et al.
2022A&A...667A..90M 45           X         1 22 ~ ArTéMiS imaging of the filamentary infrared dark clouds G1.75-0.08 and G11.36+0.80: Dust-based physical properties of the clouds and their clumps. MIETTINEN O., MATTERN M. and ANDRE P.
2024ApJ...963..126G 50           X         1 9 ~ The Magnetic Field in the Colliding Filaments G202.3+2.5. GU Q.-L., LIU T., LI P.S., et al.

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