HD 269768 , the SIMBAD biblio

HD 269768 , the SIMBAD biblio (11 results) C.D.S. - SIMBAD4 rel 1.8 - 2024.04.23CEST21:55:08


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Title First 3 Authors
1973PASP...85..439M 207 14 Red stars in the Large Magellanic Cloud. MENDOZA E.E. and GOMEZ T.
1977KodOB...2...85B 147 4 A survey of red stars in the direction of the Large Magellanic Cloud. BAPPU M.K.V., PARTHASARATHY M. and SCARIA K.K.
1977PW&SO...2..105S 1085 26 Carbon stars and late-type suspected supergiants in the LMC. SANDULEAK N. and PHILIP A.G.D.
1983A&AS...51..277R 985 48 Detection and BVR photometry of late type stars in the Large Magellanic Cloud. REBEIROT E., MARTIN N., MIANES P., et al.
1993yCat.3135....0C viz 14       D               1 252977 52 VizieR Online Data Catalog: Henry Draper Catalogue and Extension, published in Ann. Harvard Obs. 91-100 (1918-1925) CANNON A.J. and PICKERING E.C.
2015A&A...578A...3G viz 16       D               1 910 26 A new survey of cool supergiants in the Magellanic Clouds. GONZALEZ-FERNANDEZ C., DORDA R., NEGUERUELA I., et al.
2013AcA....63..159U viz 16       D               1 769 16 Variable stars from the OGLE-III Shallow Survey in the Large Magellanic Cloud. ULACZYK K., SZYMANSKI M.K., UDALSKI A., et al.
2018MNRAS.478.3138D viz 16       D               1 550 64 The luminosities of cool supergiants in the Magellanic Clouds, and the Humphreys-Davidson limit revisited. DAVIES B., CROWTHER P.A. and BEASOR E.R.
2018A&A...618A.137D viz 16       D               1 937 2 An atlas of cool supergiants from the Magellanic Clouds and typical interlopers. A guide for the classification of luminous red stars. DORDA R., NEGUERUELA I., GONZALEZ-FERNANDEZ C., et al.
2020AJ....160..120J viz 17       D               1 365761 238 APOGEE data and spectral analysis from SDSS Data Release 16: seven years of observations including first results from APOGEE-South. JONSSON H., HOLTZMAN J.A., ALLENDE PRIETO C., et al.
2021ApJ...913...32D viz 17       D               1 5182 ~ Photometric classifications of evolved massive stars: preparing for the era of webb and roman with machine learning. DORN-WALLENSTEIN T.Z., DAVENPORT J.R.A., HUPPENKOTHEN D., et al.

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