W61 28-52 , the SIMBAD biblio

W61 28-52 , the SIMBAD biblio (11 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.16CEST15:10:58


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Title First 3 Authors
1961UppAn...5a...1W 386 0 Population I in the Large Magellanic Cloud WESTERLUND B.
1973PASP...85..439M 207 14 Red stars in the Large Magellanic Cloud. MENDOZA E.E. and GOMEZ T.
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.
1985A&AS...62...23P 439 32 Radial velocities of southern stars obtained with the photoelectric scanner CORAVEL. V. 404F to M supergiant stars in the Large Magellanic Cloud. PREVOT L., ANDERSEN J., ARDEBERG A., et al.
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.
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.
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.
2022AJ....163..152S viz 17       D               1 583193 11 APOGEE Net: An Expanded Spectral Model of Both Low-mass and High-mass Stars. SPRAGUE D., CULHANE C., KOUNKEL M., et al.
2022ApJS..259...35A viz 17       D               1 611005 320 The Seventeenth Data Release of the Sloan Digital Sky Surveys: Complete Release of MaNGA, MaStar, and APOGEE-2 Data. ABDURRO'UF, ACCETTA K., AERTS C., et al.

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