[MSL2003] W43-MM3 , the SIMBAD biblio

[MSL2003] W43-MM3 , the SIMBAD biblio (21 results) C.D.S. - SIMBAD4 rel 1.8 - 2024.06.06CEST00:45:53


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Title First 3 Authors
2003ApJ...582..277M 66 160 From massive protostars to a giant H II region: submillimeter imaging of the galactic ministarburst W43. MOTTE F., SCHILKE P. and LIS D.C.
2010A&A...518L..90B 322       D     X C       8 11 49 Herschel observations of the W 43 ``mini-starburst''. BALLY J., ANDERSON L.D., BATTERSBY C., et al.
2010A&A...523A...6D 154           X C       3 127 303 A gallery of bubbles. The nature of the bubbles observed by Spitzer and what ATLASGAL tells us about the surrounding neutral material. DEHARVENG L., SCHULLER F., ANDERSON L.D., et al.
2013ApJ...775...88N 291       D     X C       7 23 93 Low-velocity shocks traced by extended SiO emission along the W43 ridges: witnessing the formation of young massive clusters. NGUYEN-LUONG Q., MOTTE F., CARLHOFF P., et al.
2014ApJ...781...89Z 42           X         1 13 93 The parallax of W43: a massive star-forming complex near the galactic bar. ZHANG B., MOSCADELLI L., SATO M., et al.
2017ApJ...839..108S viz 41           X         1 15669 21 Young stellar objects in the massive star-forming regions W51 and W43. SARAL G., HORA J.L., AUDARD M., et al.
2017A&A...601A..60C viz 41           X         1 254 18 The ATLASGAL survey: The sample of young massive cluster progenitors. CSENGERI T., BONTEMPS S., WYROWSKI F., et al.
2019ApJ...884...48C 3887     A D S   X C       92 29 ~ The seven most massive clumps in W43-Main as seen by ALMA: dynamical equilibrium and magnetic fields. CORTES P.C., HULL C.L.H., GIRART J.M., et al.
2022A&A...662A...8M 555       D     X C       12 75 20 ALMA-IMF. I. Investigating the origin of stellar masses: Introduction to the Large Program and first results. MOTTE F., BONTEMPS S., CSENGERI T., et al.
2022A&A...662A...9G viz 1451       D     X C       32 22 8 ALMA-IMF. II. Investigating the origin of stellar masses: Continuum images and data processing. GINSBURG A., CSENGERI T., GALVAN-MADRID R., et al.
2022A&A...664A..26P viz 5736 T   A D S   X C       126 8 19 ALMA-IMF. III. Investigating the origin of stellar masses: top-heavy core mass function in the
W43-MM2&
MM3
mini-starburst.
POUTEAU Y., MOTTE F., NONY T., et al.
2022A&A...665A.140B 90           X         2 24 3 ALMA-IMF. IV. A comparative study of the main hot cores in W43-MM1: Detection, temperature, and molecular composition. BROUILLET N., DESPOIS D., MOLET J., et al.
2023MNRAS.520.2306T 93           X         2 18 1 The SQUALO project (Star formation in QUiescent And Luminous Objects) I: clump-fed accretion mechanism in high-mass star-forming objects. TRAFICANTE A., JONES B.M., AVISON A., et al.
2023MNRAS.522.3548P 513           X C F     9 4 2 Will ALMA reveal the true core mass function of protoclusters? PADOAN P., PELKONEN V.-M., JUVELA M., et al.
2023A&A...674A..75N viz 4245     A D S   X C       90 8 5 ALMA-IMF V. Prestellar and protostellar core populations in the W43 cloud complex. NONY T., GALVAN-MADRID R., MOTTE F., et al.
2023A&A...674A..76P 8397 T   A D S   X C       178 24 2 ALMA-IMF VI. Investigating the origin of stellar masses: Core mass function evolution in the W43-MM2&
MM3 mini-starburst.
POUTEAU Y., MOTTE F., NONY T., et al.
2023A&A...674A.225L viz 47           X         1 9 ~ Properties of the dense cores and filamentary structures in the Vela C molecular cloud. LI X.-M., ZHANG G.-Y., MEN'SHCHIKOV A., et al.
2023MNRAS.524.1625D 112       D         F     4 21 ~ The evolution of the internal structure of massive star-forming regions in the Milky Way as revealed by ALMA. DIB S.
2023MNRAS.524.1422F 47           X         1 6 ~ The formation of globular clusters with top-heavy initial mass functions. FUKUSHIMA H. and YAJIMA H.
2023A&A...678A.194C 2165       D     X C       46 20 ~ ALMA-IMF VII. First release of the full spectral line cubes: Core kinematics traced by DCN J = (3-2). CUNNINGHAM N., GINSBURG A., GALVAN-MADRID R., et al.
2024ApJ...960...48T 970       D     X         20 20 ~ ALMA-IMF. IX. Catalog and Physical Properties of 315 SiO Outflow Candidates in 15 Massive Protoclusters. TOWNER A.P.M., GINSBURG A., DELL'OVA P., et al.

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