IRAS 18324-0737 , the SIMBAD biblio

IRAS 18324-0737 , the SIMBAD biblio (23 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.16CEST01:50:48


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Title First 3 Authors
1988IRASP.C......0J viz 14       D               1 245223 ~ Infrared Astronomical Satellite Catalogs, 1988. The Point Source Catalog, version 2.0, NASA RP-1190 JOINT IRAS SCIENCE WORKING GROUP
2000A&AS..143..269S viz 1601 191 A survey of the 6.7 GHz methanol maser emission from IRAS sources. I. Data. SZYMCZAK M., HRYNEK G. and KUS A.J.
2002A&A...392..277S 157 62 6.7 GHz methanol masers at sites of star formation. A blind survey of the Galactic plane between 20°≤l≤40° and |b|≤0.52°. SZYMCZAK M., KUS A.J., HRYNEK G., et al.
2004A&A...413..233B viz 100 24 12.2GHz survey towards 6.7GHz methanol masers. A comparison of 12.2GHz and 6.7GHz spectra. BLASZKIEWICZ L. and KUS A.J.
2005A&A...432..737P viz 942 204 A general catalogue of 6.7-GHz methanol masers. I. Data. PESTALOZZI M.R., MINIER V. and BOOTH R.S.
2006ApJ...641..389R viz 15       D               231 401 Infrared dark clouds: precursors to star clusters. RATHBORNE J.M., JACKSON J.M. and SIMON R.
2007ApJ...662.1082R 34 83 The detection of protostellar condensations in infrared dark cloud cores. RATHBORNE J.M., SIMON R. and JACKSON J.M.
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.
2008AJ....136.2391C viz 15       D               1 523 453 A catalog of extended green objects in the GLIMPSE survey: a new sample of massive young stellar object outflow candidates. CYGANOWSKI C.J., WHITNEY B.A., HOLDEN E., 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 580       D     X C       15 50 47 A comparative study of high-mass cluster forming clumps. LOPEZ-SEPULCRE A., CESARONI R. and WALMSLEY C.M.
2010ApJ...721..222B 15       D               1 54 65 An infrared through radio study of the properties and evolution of IRDC clumps. BATTERSBY C., BALLY J., JACKSON J.M., 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 132       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.
2017ApJS..232....3W viz 254       D S   X         6 52 13 Deep, broadband spectral line surveys of molecule-rich interstellar clouds. WIDICUS WEAVER S.L., LAAS J.C., ZOU L., et al.
2019AJ....158...18H 219       D     X         6 23 ~ APEX millimeter observations of methanol emission toward high-mass star-forming cores. HERNANDEZ-HERNANDEZ V., KURTZ S., KALENSKII S., et al.
2020ApJ...897L..38V viz 16       D               1 83 15 Carbon-grain sublimation: a new top-down component of protostellar chemistry. VAN 'T HOFF M.L.R., BERGIN E.A., JORGENSEN J.K., et al.
2021A&A...645A..29K 435       D     X C       10 41 4 Search for radio jets from massive young stellar objects. Association of radio jets with H2O and CH3OH masers. KAVAK U., SANCHEZ-MONGE A., LOPEZ-SEPULCRE A., et al.
2021MNRAS.504..338P viz 184       D     X   F     4 134 17 A Galactic survey of radio jets from massive protostars. PURSER S.J.D., LUMSDEN S.L., HOARE M.G., et al.
2023ApJ...954..189S 44           X         1 43 ~ Survey of CH3NH2 and its Formation Process. SUZUKI T., MAJUMDAR L., GOLDSMITH P.F., et al.
2023A&A...679A.123K viz 627       D     X         15 37 ~ A survey of SiO J = 1-0 emission toward massive star-forming regions. KIM W.-J., URQUHART J.S., VEENA V.S., et al.
2023RNAAS...7..258S 261           X C       5 2 ~ On the Chromaticity of the (NEO)WISE Astrometry. STECKLUM B.

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