JCMTSE J064118.0+092902 , the SIMBAD biblio

JCMTSE J064118.0+092902 , the SIMBAD biblio (10 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.19CEST00:25:43


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Title First 3 Authors
2006A&A...445..979P 52 147 Probing the formation of intermediate- to high-mass stars in protoclusters. A detailed millimeter study of the NGC 2264 clumps. PERETTO N., ANDRE P. and BELLOCHE A.
2006A&A...455..903F viz 1178 74 ACIS-I observations of NGC 2264. Membership and X-ray properties of PMS stars. FLACCOMIO E., MICELA G. and SCIORTINO S.
2007A&A...464..983P 1 18 69 Probing the formation of intermediate- to high-mass stars in protoclusters. II. Comparison between millimeter interferometric observations of NGC 2264-C and SPH simulations of a collapsing clump. PERETTO N., HENNEBELLE P. and ANDRE P.
2008ApJS..175..277D viz 15       D               7164 308 The SCUBA legacy catalogues: submillimeter-continuum objects detected by SCUBA. DI FRANCESCO J., JOHNSTONE D., KIRK H., et al.
2009A&A...499..175M viz 539       D     X C F     13 39 25 Probing the role of protostellar feedback in clustered star formation. Mapping outflows in the collapsing protocluster NGC 2264-C. MAURY A.J., ANDRE P. and LI Z.-Y.
2012MNRAS.423.1127B 282       D     X   F     7 47 5 The structure of molecular gas associated with NGC 2264: wide-field 12CO and H2imaging. BUCKLE J.V., RICHER J.S. and DAVIS C.J.
2012A&A...544A..69M viz 76               F     1 17 2 CN Zeeman observations of the NGC 2264-C protocluster. MAURY A.J., WIESEMEYER H. and THUM C.
2015MNRAS.453.2006B viz 16       D               1 146 1 Wide-field SCUBA-2 observations of NGC 2264: submillimetre clumps and filaments. BUCKLE J.V. and RICHER J.S.
2021A&A...645A..94N viz 17       D               1 277 20 Mass segregation and sequential star formation in NGC 2264 revealed by Herschel. NONY T., ROBITAILLE J.-F., MOTTE F., et al.
2021ApJ...918...32S 42           X         1 19 ~ Exploring the 100 au scale structure of the protobinary system NGC 2264 CMM3 with ALMA. SHIBAYAMA Y., WATANABE Y., OYA Y., et al.

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