SK -67 54 , the SIMBAD biblio

SK -67 54 , the SIMBAD biblio (11 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.16CEST22:18:59


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Title First 3 Authors
1970CoTol..89....1S viz 1286 ~ A deep objective-prism survey for Large Magellanic Cloud members. SANDULEAK N.
1972A&AS....6..249A 630 199 Spectrographic and photometric observations of supergiants and foreground stars, in the direction of the Large Magellanic Cloud. ARDEBERG A., BRUNET J.P., MAURICE E., et al.
1974A&AS...13..173F 1902 22 Vitesses radiales au prisme-objectif dans la direction du Grand Nuage de Magellan. Liste de 398 etoiles, membres du GNM. Liste de 1434 etoiles galactiques en direction du GNM. FEHRENBACH C. and DUFLOT M.
1982A&AS...48..409F 1270 22 Vitesses radiales au prisme objectif dans la direction du Grand Nuage de Magellan. FEHRENBACH C. and DUFLOT M.
1999A&AS..139..277H viz 814 71 A ROSAT PSPC catalogue of X-ray sources in the LMC region. HABERL F. and PIETSCH W.
2001PASP..113.1130J 61 13 Spectroscopic classification of 42 Large Magellanic Cloud OB stars: selection of probes for the hot gaseous halo of the Large Magellanic Cloud. JAXON E.G., GUERRERO M.A., HOWK J.C., 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.
2013A&A...555A.141H viz 15       D               1 1714 3 Emission-line stars in the LMC: the Armagh survey and a metacatalogue. HOWARTH I.D.
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...676A..85S 17       D               2 127 ~ The ESO UVES/FEROS Large Programs of TESS OB pulsators I. Global stellar parameters from high-resolution spectroscopy. SEREBRIAKOVA N., TKACHENKO A., GEBRUERS S., et al.
2024A&A...692A.245S viz 18       D               1 192 ~ The ESO UVES/FEROS Large Programs of TESS OB pulsators II. The physical origin of macroturbulence. SEREBRIAKOVA N., TKACHENKO A. and AERTS C.

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