2MASS J05351519-0522367 , the SIMBAD biblio

2MASS J05351519-0522367 , the SIMBAD biblio (24 results) C.D.S. - SIMBAD4 rel 1.8 - 2024.04.25CEST03:37:12


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Title First 3 Authors
1982AJ.....87.1819L 29 56 New members of the infrared cluster in the Orion molecular cloud. LONSDALE C.J., BECKLIN E.E., LEE T.J., et al.
1999AJ....117.1375S viz 315 96 Adaptive optics imaging of the Orion Trapezium cluster. SIMON M., CLOSE L.M. and BECK T.L.
2000AJ....120.3162L 100 191 Infrared l-band observations of the Trapezium cluster: a census of circumstellar disks and candidate protostars. LADA C.J., MUENCH A.A., HAISCH K.E.Jr, et al.
2000ApJ...540..236H viz 831 286 Constraints on the stellar/substellar mass function in the inner Orion nebula cluster. HILLENBRAND L.A. and CARPENTER J.M.
2000ApJ...540.1016L viz 346 241 The initial mass function of low-mass stars and brown dwarfs in young clusters. LUHMAN K.L., RIEKE G.H., YOUNG E.T., et al.
2002ApJ...573..366M viz 1054 350 The luminosity and mass function of the Trapezium cluster: from B stars to the deuterium-burning limit. MUENCH A.A., LADA E.A., LADA C.J., et al.
2004AJ....128.1254L viz 466 55 Deep 3.8 micron observations of the Trapezium cluster. LADA C.J., MUENCH A.A., LADA E.A., et al.
2005AJ....129.1534R viz 15       D               256 40 The Orion nebula in the mid-infrared. ROBBERTO M., BECKWITH S.V.W., PANAGIA N., et al.
2005ApJS..160..319G viz 15       D               1 2038 330 Chandra Orion Ultradeep Project: observations and sources lists. GETMAN K.V., FLACCOMIO E., BROOS P.S., et al.
2007A&A...466..949N viz 59 22 Observations of spatial and velocity structure in the Orion molecular cloud. NISSEN H.D., GUSTAFSSON M., LEMAIRE J.L., et al.
2016ApJ...826...16E viz 16       D               1 314 27 Protoplanetary disks in the Orion OMC1 region imaged with ALMA. EISNER J.A., BALLY J.M., GINSBURG A., et al.
2016ApJ...831..155S viz 16       D               1 927 3 A VLA survey for faint compact radio sources in the Orion Nebula Cluster. SHEEHAN P.D., EISNER J.A., MANN R.K., et al.
2017ApJ...838L...3L 1609     A     X C       39 10 17 New evidence for the dynamical decay of a multiple system in the Orion Kleinmann-Low Nebula. LUHMAN K.L., ROBBERTO M., TAN J.C., et al.
2017ApJ...850..158S 81           X         2 13 1 A molecular-line study of the interstellar bullet engine IRAS 05506+2414. SAHAI R., LEE C.-F., SANCHEZ CONTRERAS C., et al.
2018A&A...612L...7F 535           X C       12 5 3 On the formation of runaway stars BN and x in the Orion Nebula Cluster. FARIAS J.P. and TAN J.C.
2018ApJ...860...77E 16       D               1 239 99 Protoplanetary disk properties in the Orion Nebula Cluster: initial results from deep, high-resolution ALMA observations. EISNER J.A., ARCE H.G., BALLERING N.P., et al.
2018ApJ...865L..18I 123           X         3 9 1 High spectral resolution observations toward Orion BN at 6 µm: no evidence for hot water. INDRIOLO N., TAN J.C., BOOGERT A.C.A., et al.
2019AJ....157..109K viz 669           X C       15 14 8 Stellar proper motions in the Orion Nebula Cluster. KIM D., LU J.R., KONOPACKY Q., et al.
2019A&A...626A..79P viz 17       D               1 1887 ~ Do star clusters form in a completely mass-segregated way? PAVLIK V., KROUPA P. and SUBR L.
2020ApJ...889..178B 2128     A D S   X C       49 16 ~ The Orion protostellar explosion and runaway stars revisited: stellar masses, disk retention, and an outflow from the Becklin-Neugebauer object. BALLY J., GINSBURG A., FORBRICH J., et al.
2020ApJ...892...82R 894     A D     X C       21 15 ~ Proper motions of the radio source Orion MR, formerly known as Orion n, and new sources with large proper motions in Orion BN/KL. RODRIGUEZ L.F., DZIB S.A., ZAPATA L., et al.
2020MNRAS.495.1172D 255           X         6 10 ~ Formation of Orion fingers. DEMPSEY R., ZAKAMSKA N.L. and OWEN J.E.
2021ApJ...907...94C 88               F     1 12 13 The explosion in Orion-KL as seen by mosaicking the magnetic field with ALMA. CORTES P.C., LE GOUELLEC V.J.M., HULL C.L.H., et al.
2021ApJ...916...56R 6 ~ Explosive ejections generated by gravitational interactions. RIVERA-ORTIZ P.R., RODRIGUEZ-GONZALEZ A., CANTO J., et al.

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