NAME Nessie Nebula , the SIMBAD biblio

NAME Nessie Nebula , the SIMBAD biblio (26 results) C.D.S. - SIMBAD4 rel 1.8 - 2023.06.04CEST09:14:41


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Title First 3 Authors
2010ApJ...719L.185J 1447     A     X C       37 16 101 The "
Nessie" nebula: cluster formation in a filamentary infrared dark cloud.
JACKSON J.M., FINN S.C., CHAMBERS E.T., et al.
2012A&A...540L..11S 42           X         1 24 191 Cluster-formation in the Rosette molecular cloud at the junctions of filaments. SCHNEIDER N., CSENGERI T., HENNEMANN M., et al.
2012A&A...542A.101M viz 39           X         1 164 15 LABOCA 870 µm dust continuum mapping of selected infrared-dark cloud regions in the Galactic plane. MIETTINEN O.
2013MNRAS.433..251C 330       D     X C       8 17 23 Structure and radial equilibrium of filamentary molecular clouds. CONTRERAS Y., RATHBORNE J. and GARAY G.
2013A&A...559A..34L 158           X C       3 11 24 A 500 pc filamentary gas wisp in the disk of the Milky Way. LI G.-X., WYROWSKI F., MENTEN K., et al.
2014A&A...562A...3M 79           X         2 57 25 A MALT90 study of the chemical properties of massive clumps and filaments of infrared dark clouds. MIETTINEN O.
2014A&A...568A..73R 652       D     X         17 27 59 Giant molecular filaments in the Milky Way. RAGAN S.E., HENNING T., TACKENBERG J., et al.
2012A&ARv..20...55H 44           X         1 14 162 Turbulent molecular clouds. HENNEBELLE P. and FALGARONE E.
2014MNRAS.444..336C 41           X         1 8 26 Filamentary star formation in NGC 1275. CANNING R.E.A., RYON J.E., GALLAGHER III J.S., et al.
2014ApJ...797...53G 5563     A D     X C       140 7 48 The bones of the Milky Way. GOODMAN A.A., ALVES J., BEAUMONT C.N., et al.
2015MNRAS.450.4043W 901       D     X C F     21 25 53 Large-scale filaments associated with Milky Way spiral arms. WANG K., TESTI L., GINSBURG A., et al.
2015ApJ...815...23Z 867     A     X C       21 30 21 The skeleton of the Milky Way. ZUCKER C., BATTERSBY C. and GOODMAN A.
2016MNRAS.456.2041C viz 41           X         1 102 22 Fragmentation in filamentary molecular clouds. CONTRERAS Y., GARAY G., RATHBORNE J.M., et al.
2016MNRAS.458.1815W 41           X         1 6 1 A ram-pressure threshold for star formation. WHITWORTH A.P.
2016A&A...591A...5L viz 341       D     X C       8 42 30 ATLASGAL: A Galaxy-wide sample of dense filamentary structures. LI G.-X., URQUHART J.S., LEURINI S., et al.
2016ApJ...825..125P 41           X         1 27 14 Rapid circumstellar disk evolution and an accelerating star formation rate in the infrared dark cloud M17 SWex. POVICH M.S., TOWNSLEY L.K., ROBITAILLE T.P., et al.
2018A&A...609A.123M viz 167           X         4 23 2 The Seahorse Nebula: New views of the filamentary infrared dark cloud G304.74+01.32 from SABOCA, Herschel, and WISE. MIETTINEN O.
2018A&A...610A..77H viz 42           X         1 45 10 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.
2018A&A...616A..78M viz 4038 T   A S   X C       94 7 1 Structure and fragmentation of a high line-mass filament:
Nessie.
MATTERN M., KAINULAINEN J., ZHANG M., et al.
2019A&A...622A..52Z 17       D               2 81 ~ Star-forming content of the giant molecular filaments in the Milky Way. ZHANG M., KAINULAINEN J., MATTERN M., et al.
2020MNRAS.492.1594S 157     A     X         4 4 ~ The Cloud Factory I: Generating resolved filamentary molecular clouds from galactic-scale forces. SMITH R.J., TRESS R.G., SORMANI M.C., et al.
2019PASJ...71S...3N 43           X         1 33 ~ Nobeyama 45 m mapping observations toward the nearby molecular clouds Orion A, Aquila Rift, and M17: Project overview. NAKAMURA F., ISHII S., DOBASHI K., et al.
2021ApJ...918L...2L 179           X         4 8 ~ The discovery of the largest gas filament in our Galaxy, or a new spiral arm? LI C., QIU K., HU B., et al.
2021ApJ...921...23G 45           X         1 27 ~ A wide-field CO survey toward the California molecular filament. GUO W., CHEN X., FENG J., et al.
2022MNRAS.517.4679K 93           X         2 7 ~ Filament formation via collision-induced magnetic reconnection - formation of a star cluster. KONG S., WHITWORTH D.J., SMITH R.J., et al.
2022A&A...667A..90M 47           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.

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2023.06.04-09:14:41

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