[RJS2006] MSXDC G025.04-00.20 MM1 , the SIMBAD biblio

[RJS2006] MSXDC G025.04-00.20 MM1 , the SIMBAD biblio (10 results) C.D.S. - SIMBAD4 rel 1.8 - 2024.04.18CEST23:24:04

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Bibcode/DOI Score in Title|Abstract|
Keywords 		in a table in teXt, Caption, ... Nb occurence Nb objects in ref Citations
(from ADS) 		Title First 3 Authors
2006ApJ...641..389R viz 15       D               231 401 Infrared dark clouds: precursors to star clusters. RATHBORNE J.M., JACKSON J.M. and SIMON R.
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.
2009ApJS..181..360C 224 183 Star formation activity of cores within infrared dark clouds. CHAMBERS E.T., JACKSON J.M., RATHBORNE J.M., et al.
2010ApJ...715..310R viz 15       D               1 194 84 The early stages of star formation in infrared dark clouds: characterizing the core dust properties. RATHBORNE J.M., JACKSON J.M., CHAMBERS E.T., et al.
2010A&A...517A..66L 511       D     X C       13 50 47 A comparative study of high-mass cluster forming clumps. LOPEZ-SEPULCRE A., CESARONI R. and WALMSLEY C.M.
2011A&A...526L...2L 15       D               2 60 33 SiO outflows in high-mass star forming regions: a potential chemical clock? LOPEZ-SEPULCRE A., WALMSLEY C.M., CESARONI R., et al.
2012ApJ...756...60S viz 15       D               1 198 159 Chemistry in infrared dark cloud clumps: a molecular line survey at 3 mm. SANHUEZA P., JACKSON J.M., FOSTER J.B., et al.
2014A&A...570A..49L viz 134       D     X         4 21 10 SiO excitation from dense shocks in the earliest stages of massive star formation. LEURINI S., CODELLA C., LOPEZ-SEPULCRE A., et al.
2016ApJS..227...25R viz 16       D               2 77 58 Weak and compact radio emission in early high-mass star-forming regions. I. VLA observations. ROSERO V., HOFNER P., CLAUSSEN M., et al.
2019ApJ...880...99R 64 22 Weak and compact radio emission in early high-mass star-forming regions. II. The nature of the radio sources. ROSERO V., HOFNER P., KURTZ S., et al.

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