IRAS 05195-6911 , the SIMBAD biblio

IRAS 05195-6911 , the SIMBAD biblio (20 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.16CEST14:08:00


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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
2001AJ....122.1844E viz 1825 79 MSX, 2MASS, and the Large Magellanic Cloud: a combined near- and mid-infrared view. EGAN M.P., VAN DYK S.D. and PRICE S.D.
2004AJ....128.2206I 161 26 Australia telescope compact array survey of candidate ultracompact and buried H II regions in the Magellanic Clouds. INDEBETOUW R., JOHNSON K.E. and CONTI P.
2008AJ....136...18W viz 15       D               1 1226 186 Spitzer SAGE survey of the Large Magellanic Cloud. III. Star formation and ∼1000 new candidate young stellar objects. WHITNEY B.A., SEWILO M., INDEBETOUW R., et al.
2008AJ....136.1221K viz 15       D               2 280 28 The Large Magellanic Cloud's top 250: classification of the most luminous compact 8 µm sources in the Large Magellanic Cloud. KASTNER J.H., THORNDIKE S.L., ROMANCZYK P.A., et al.
2009ApJ...699..150S viz 15       D               1 295 80 The evolution of massive young stellar objects in the large Magellanic cloud. I. Identification and spectral classification. SEALE J.P., LOONEY L.W., CHU Y.-H., et al.
2009ApJS..184..172G viz 15       D               1 2912 133 High- and intermediate-mass young stellar objects in the Large Magellanic Cloud. GRUENDL R.A. and CHU Y.-H.
2009AJ....138.1597B 15       D               2 72 17 Spitzer IRS spectra of luminous 8 µm sources in the large Magellanic cloud: testing color-based classifications. BUCHANAN C.L., KASTNER J.H., HRIVNAK B.J., et al.
2016A&A...585A.107S 16       D               1 31 9 VLT/ISAAC infrared spectroscopy of embedded high-mass YSOs in the Large Magellanic Cloud: Methanol and the 3.47 µm band. SHIMONISHI T., DARTOIS E., ONAKA T., et al.
2018ApJ...854...13P 16       D               1 32 2 Modeling CO, CO2, and H2O ice abundances in the envelopes of young stellar objects in the Magellanic Clouds. PAULY T. and GARROD R.T.
2020ApJ...891..164S 2593     A D S   X C       62 11 ~ Chemistry and physics of a low-metallicity hot core in the Large Magellanic Cloud. SHIMONISHI T., DAS A., SAKAI N., et al.
2021ApJ...922..206S 543           X C       12 15 12 The detection of a hot molecular core in the extreme outer Galaxy. SHIMONISHI T., IZUMI N., FURUYA K., et al.
2022ApJ...931..102S 468           X C       10 55 6 ALMA Observations of Molecular Complexity in the Large Magellanic Cloud: The N 105 Star-forming Region. SEWILO M., CORDINER M., CHARNLEY S.B., et al.
2023ApJ...955...52T 148       D     X         4 89 ~ An ALMA Glimpse of Dense Molecular Filaments Associated with High-mass Protostellar Systems in the Large Magellanic Cloud. TOKUDA K., HARADA N., TANAKA K.E.I., et al.
2024A&A...688A...3G 645       D     X C       14 35 ~ High-mass star formation across the Large Magellanic Cloud I. Chemical properties and hot molecular cores observed with ALMA at 1.2 mm. GOLSHAN R.H., SANCHEZ-MONGE A., SCHILKE P., et al.
2025ApJ...988..111I 187           X         4 9 ~ The Detection of Spatially Resolved Protostellar Outflows and Episodic Jets in the Outer Galaxy. IKEDA T., SHIMONISHI T., IZUMI N., et al.
2025ApJ...991...59B 280           X C       5 35 ~ ALMA Observations of Molecular Complexity in the Large Magellanic Cloud: Probing the Star-forming Region N 160. BROADMEADOW A., SEWILO M., MUNDY L., et al.
2025A&A...704A..31G 93             C       1 21 ~ Probing sulphur chemistry in oxygen-rich asymptotic giant branch stars with ALMA. GORAI P., SABERI M., KHOURI T., et al.
2026ApJS..282...64S 20       D               1 17 ~ Magellanic Outflow and Chemistry Survey (MAGOS): Hot Cores in the LMC. SHIMONISHI T., TANAKA K.E.I., ZHANG Y., et al.
2026ApJ...998..277M 370       D     X         8 23 ~ ALMA Observations of Cold Methanol Gas in the Large Magellanic Cloud: N79 South Giant Molecular Cloud. MONDAL S.K., SHIMONISHI T., MONDAL S., et al.

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