JCMTSF J053526.4-050521 , the SIMBAD biblio

JCMTSF J053526.4-050521 , the SIMBAD biblio (25 results) C.D.S. - SIMBAD4 rel 1.7 - 2021.05.13CEST00:00:04


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Title First 3 Authors
2021ApJ...910..148M 50           X         1 21 ~ Revealing a centrally condensed structure in OMC-3/MMS 3 with ALMA high-resolution observations. MORII K., TAKAHASHI S. and MACHIDA M.N.
2020MNRAS.497..793Z 187             C F     3 22 ~ Filament intersections and cold dense cores in Orion A North. ZHANG C., REN Z., WU J., et al.
2019PASJ...71S...8T 179           X         4 45 ~ Nobeyama 45 m mapping observations toward Orion A. I. Molecular outflows. TANABE Y., NAKAMURA F., TSUKAGOSHI T., et al.
2018A&A...610A..77H viz 44           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.
2017A&A...600A.141K viz 170           X C       3 70 26 Resolving the fragmentation of high line-mass filaments with ALMA: the integral shaped filament in Orion A. KAINULAINEN J., STUTZ A.M., STANKE T., et al.
2016A&A...588A..30S viz 17       D               1 24 12 Dust emissivity in the star-forming filament OMC 2/3. SADAVOY S.I., STUTZ A.M., SCHNEE S., et al.
2010ApJ...710.1247S viz 16       D               1 761 82 The mass distribution of starless and protostellar cores in Gould Belt clouds. SADAVOY S.I., DI FRANCESCO J., BONTEMPS S., et al.
2010ApJ...716..893P viz 445       D     X   F     11 42 25 Magnetic field structures and turbulent components in the star-forming molecular clouds OMC-2 and OMC-3. POIDEVIN F., BASTIEN P. and MATTHEWS B.C.
2008A&A...487..605A 15       D               1 75 10 The direction of outflows from filaments: constraints on core formation. ANATHPINDIKA S. and WHITWORTH A.P.
2008ApJ...688..344T 92       D       C       3 61 25 Millimeter- and submillimeter-wave observations of the OMC-2/3 region. III. An extensive survey for molecular outflows. TAKAHASHI S., SAITO M., OHASHI N., et al.
2008ApJS..175..277D viz 15       D               7196 197 The SCUBA legacy catalogues: submillimeter-continuum objects detected by SCUBA. DI FRANCESCO J., JOHNSTONE D., KIRK H., et al.
2008PASJ...60..407T 15       D     X         1 59 26 N2H+ and HC3N observations of the Orion A cloud. TATEMATSU K., KANDORI R., UMEMOTO T., et al.
2004ApJ...604..717H viz 1 23 68 Tracing the magnetic field in Orion A. HOUDE M., DOWELL C.D., HILDEBRAND R.H., et al.
2003ApJ...591.1025W 31 45 High-resolution imaging of CO outflows in OMC-2 and OMC-3. WILLIAMS J.P., PLAMBECK R.L. and HEYER M.H.
2002ApJ...573..270T 36 7 Deep near-infrared observations of the x-ray-emitting class 0 protostar candidates in the Orion molecular cloud 3. TSUJIMOTO M., KOYAMA K., TSUBOI Y., et al.
2001ApJ...562..400M 23 66 Magnetic fields in star-forming molecular clouds. II. The depolarization effect in the OMC-3 filament of Orion A. MATTHEWS B.C., WILSON C.D. and FIEGE J.D.
2000AJ....120.1974Y 128 44 A multiwavelength study of outflows in OMC-2/3. YU K.C., BILLAWALA Y., SMITH M.D., et al.
2000AcApS..20..403S 21 0 Molecular radiation of 13CO (J = 1 - 0) and C18O (J = 1 - 0) from OMC-3. SUN J., SONG L.-M., ZHANG Y.-P., et al.
2000ApJ...531..868M 1 17 56 Magnetic fields in star-forming molecular clouds. I. The first polarimetry of OMC-3 in Orion A. MATTHEWS B.C. and WILSON C.D.
2000ApJ...533..440G 56 45 Does infall end before the class I stage? GREGERSEN E.M., EVANS II N.J., MARDONES D., et al.
2000ApJS..131..465A 65 48 Dense cores and molecular outflows in the OMC-2/3 region. ASO Y., TATEMATSU K., SEKIMOTO Y., et al.
1999ApJ...510L..49J 2 25 198 JCMT/SCUBA submillimeter wavelength imaging of the integral-shaped filament in Orion. JOHNSTONE D. and BALLY J.
1998ApJ...509..299L 1 45 147 350 micron continuum imaging of the Orion A molecular cloud with the submillimeter high angular resolution camera. LIS D.C., SERABYN E., KEENE J., et al.
1997ApJ...474L.135C 1 27 136 Dust filaments and star formation in OMC-2 and OMC-3. CHINI R., REIPURTH B., WARD-THOMPSON D., et al.
1997ApJ...485L..45Y 120 60 Shock-excited H2 flows in OMC-2 and OMC-3. YU K.C., BALLY J. and DEVINE D.

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2021.05.13-00:00:04

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