SK -67 261 , the SIMBAD biblio

SK -67 261 , the SIMBAD biblio (10 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.15CEST15:37:33


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Title First 3 Authors
1970CoTol..89....1S viz 13       D               1286 ~ A deep objective-prism survey for Large Magellanic Cloud members. SANDULEAK N.
1972A&A....21..329M 98 5 Developpement de la technique du prisme-objectif: recherche, d'etoiles faibles appartenant au Grand Nuage de Magellan. MARTIN N. and REBEIROT E.
1977A&A....58..209M 86 8 Uvby photometry of very hot stars in the Large Magellanic Cloud. MIANES P., PREVOT L., PREVOT-BURNICHON M.L., et al.
1995ApJ...438..188M 308 381 Massive stars in the field and associations of the Magellanic Clouds : the upper mass limit, the initial mass function and a critical test of main-sequence stellar evolutionary theory. MASSEY P., LANG C.C., DE GIOIA-EASTWOOD K., et al.
2009AJ....138.1003B viz 15       D               1 1760 163 Spitzer SAGE infrared photometry of massive stars in the Large Magellanic Cloud. BONANOS A.Z., MASSA D.L., SEWILO M., 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.
2023ApJ...952...64L viz 17       D               1 2632 ~ Massive Hypervelocity Runaway Stars in the Large Magellanic Cloud. LIN Z., XU Y., HAO C., et al.
2023A&A...675A.154V viz 17       D               1 256 ~ X-Shooting ULLYSES: Massive stars at low metallicity I. Project description. VINK J.S., MEHNER A., CROWTHER P.A., et al.
2024A&A...689A..31M 197       D     X C       4 155 ~ X-Shooting ULLYSES: Massive stars at low metallicity V. Effect of metallicity on surface abundances of O stars. MARTINS F., BOURET J.-C., HILLIER D.J., et al.
2025A&A...695A.198B viz 19       D               1 247 ~ X-Shooting ULLYSES: Massive stars at low metallicity XI. Pipeline-determined physical properties of Magellanic Cloud OB stars. BESTENLEHNER J.M., CROWTHER P.A., HAWCROFT C., et al.

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