MSX LMC 787 , the SIMBAD biblio

MSX LMC 787 , the SIMBAD biblio (10 results) C.D.S. - SIMBAD4 rel 1.8 - 2024.04.19CEST15:31:47

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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
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.
2008ApJ...681.1557L 15       D               3 120 29 Effects of metallicity on the chemical composition of carbon stars. LEISENRING J.M., KEMPER F. and SLOAN G.C.
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.
2009A&A...506.1277G viz 15       D               1 231 158 Luminosities and mass-loss rates of SMC and LMC AGB stars and red supergiants. GROENEWEGEN M.A.T., SLOAN G.C., SOSZYNSKI I., et al.
2011A&A...530A..90V viz 15       D               1 1414 46 The optically bright post-AGB population of the LMC. VAN AARLE E., VAN WINCKEL H., LLOYD EVANS T., et al.
2016ApJ...826...44S viz 16       D               1 237 24 The infrared spectral properties of Magellanic carbon stars. SLOAN G.C., KRAEMER K.E., McDONALD I., et al.
2018A&A...609A.114G viz 16       D               1 408 55 Luminosities and mass-loss rates of Local Group AGB stars and red supergiants. GROENEWEGEN M.A.T. and SLOAN G.C.
2019A&A...626A..92G viz 393       D     X C       9 225 ~ 30-micron sources in galaxies with different metallicities. GLADKOWSKI M., SZCZERBA R., SLOAN G.C., et al.
2019ApJ...887...82K viz 17       D               1 263 ~ Stellar pulsation and the production of dust and molecules in galactic carbon stars. KRAEMER K.E., SLOAN G.C., KELLER L.D., et al.
2020A&A...636A..48G viz 17       D               3 970 ~ 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.

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