MSX LMC 941 , the SIMBAD biblio

MSX LMC 941 , the SIMBAD biblio (10 results) C.D.S. - SIMBAD4 rel 1.8 - 2024.04.18CEST02:45:19


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Title First 3 Authors
2001AJ....122.1844E viz 1826 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.
2004A&A...425..595G viz 2919 66 Long Period Variables in the Magellanic Clouds: OGLE + 2MASS + DENIS. GROENEWEGEN M.A.T.
2008AJ....136.1221K viz 15       D               1 280 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.
2009AJ....137.3139V viz 15       D               1 1973 42 Variable evolved stars and young stellar objects discovered in the large Magellanic cloud using the SAGE survey. VIJH U.P., MEIXNER M., BABLER B., 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.
2009AcA....59..239S viz 15       D               1 46478 185 The Optical Gravitational Lensing Experiment. The OGLE-III catalog of variable stars. IV. Long-period variables in the Large Magellanic Cloud. SOSZYNSKI I., UDALSKI A., SZYMANSKI M.K., et al.
2017AJ....154..149Y viz 16       D               1 692 33 Large Magellanic Cloud near-infrared synoptic survey. V. Period-Luminosity relations of Miras. YUAN W., MACRI L.M., HE S., et al.
2020A&A...636A..48G viz 17       D               1 970 ~ The VMC Survey. XXXVII. Pulsation periods of dust-enshrouded AGB stars in the Magellanic Clouds. GROENEWEGEN M.A.T., NANNI A., CIONI M.-R.L., et al.
2021ApJ...919...99I viz 17       D               1 1667 10 Mid-infrared period-luminosity relations for Miras in the Large Magellanic Cloud. IWANEK P., SOSZYNSKI I. and KOZLOWSKI S.
2021A&A...656A..66T viz 17       D               1 14341 8 Semi-regular red giants as distance indicators. I. The period-luminosity relations of semi-regular variables revisited. TRABUCCHI M., MOWLAVI N. and LEBZELTER T.

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