NAME Orion Southern Filament , the SIMBAD biblio

NAME Orion Southern Filament , the SIMBAD biblio (12 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.17CEST07:10:24

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Bibcode/DOI Score in Title|Abstract|
Keywords 		in a table in teXt, Caption, ... Nb occurence Nb objects in ref Citations
(from ADS) 		Title First 3 Authors
1986ApJ...303..375M 161 357 The large system of molecular clouds in Orion and Monoceros. MADDALENA R.J., MORRIS M., MOSCOWITZ J., et al.
1987ApJ...312L..45B 7 14 534 Filamentary structure in the Orion molecular cloud. BALLY J., LANGER W.D., STARK A.A., et al.
1989ARA&A..27...41G 9 13 492 The Orion molecular cloud and star-forming region. GENZEL R. and STUTZKI J.
2000MNRAS.311...85F 6 14 271 Helical fields and filamentary molecular clouds - I. FIEGE J.D. and PUDRITZ R.E.
2003AJ....126.2971V viz 203 221 Investigation of 131 Herbig Ae/Be candidate stars. VIEIRA S.L.A., CORRADI W.J.B., ALENCAR S.H.P., et al.
2004PASJ...56..313K viz 207 15 13^CO (J = 1-0) survey toward of molecular clouds toward the Monoceros and Canis Major Region. KIM B.G., KAWAMURA A., YONEKURA Y., et al.
2007AJ....133.2192H 37   K                 28 21 Large-scale flows from
Orion South. 		HENNEY W.J., O'DELL C.R., ZAPATA L.A., et al.
2009A&A...504..451A 38           X         1 3 7 Supersonic cloud collision - II. ANATHPINDIKA S.
2017ApJS..228...12T 40           X         1 91 19 Astrochemical properties of Planck cold clumps. TATEMATSU K., LIU T., OHASHI S., et al.
2017ApJ...845..105D 40           X         1 15 27 IN-SYNC. V. Stellar kinematics and dynamics in the Orion A molecular cloud. DA RIO N., TAN J.C., COVEY K.R., et al.
2018ApJS..235...15L viz 40           X         1 30 3 Molecular gas toward the Gemini OB1 molecular cloud complex. II. CO Outflow candidates with possible WISE associations. LI Y., LI F.-C., XU Y., et al.
2023A&A...670A.151Y 44           X         1 22 1 The most massive stars in very young star clusters with a limited mass: Evidence favours significant self-regulation in the star formation processes. YAN Z., JERABKOVA T. and KROUPA P.

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