BGPSv2 G018.655-00.060 , the SIMBAD biblio

BGPSv2 G018.655-00.060 , the SIMBAD biblio (10 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.16CEST23:46:46


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Title First 3 Authors
2002ApJ...566..945B viz 14       D               1 198 433 High-mass protostellar candidates. II. Density structure from dust continuum and CS emission. BEUTHER H., SCHILKE P., MENTEN K.M., et al.
2004A&A...417..115W viz 114 84 The circumstellar environments of high-mass protostellar objects. I. Submillimetre continuum emission. WILLIAMS S.J., FULLER G.A. and SRIDHARAN T.K.
2008A&A...479..751T 15       D               4 115 10 The circumstellar environment of high-mass protostellar objects. IV. C17O observations and depletion. THOMAS H.S. and FULLER G.A.
2008ApJ...678.1049S 15       D               1 65 68 A molecular line observation toward massive clumps associated with infrared dark clouds. SAKAI T., SAKAI N., KAMEGAI K., et al.
2010ApJ...714.1658S 15       D               1 25 29 A survey of molecular lines toward massive clumps in early evolutionary stages of high-mass star formation. SAKAI T., SAKAI N., HIROTA T., et al.
2011ApJ...743..196C 15       D               1 22 18 Deuterium fractionation as an evolutionary probe in massive Protostellar/Cluster cores. CHEN H.-R., LIU S.-Y., SU Y.-N., et al.
2012ApJ...747..140S 244       D     X   F     6 22 26 DNC/HNC ratio of massive clumps in early evolutionary stages of high-mass star formation. SAKAI T., SAKAI N., FURUYA K., et al.
2015A&A...576A.131H 16       D               1 77 2 Combination of CN(1-0), HCN(1-0), and HNC(1-0): A possible indicator for a high-mass star formation sequence in the Milky Way. HAN X.H., ZHOU J.J., WANG J.Z., et al.
2017MNRAS.471..100E viz 16       D               1 62449 117 The Hi-GAL compact source catalogue - I. The physical properties of the clumps in the inner Galaxy (-71.0° < l < 67.0°). ELIA D., MOLINARI S., SCHISANO E., et al.
2018ApJ...854..133T 16       D               1 76 10 Survey observations to study chemical evolution from high-mass starless cores to high-mass protostellar objects. I. HC3N and HC5N. TANIGUCHI K., SAITO M., SRIDHARAN T.K., et al.

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