SK -69 212 , the SIMBAD biblio

SK -69 212 , the SIMBAD biblio (22 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.14CEST09:58:17


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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.
1984A&A...139..330L 14 31 Optical observations of the bubble nebula N 157C (=0536.6-6914) and the tight clusters in the association LH 90 in LMC. LORTET M.C. and TESTOR G.
1986AJ.....92...48C 244 119 Studies of massive stars in the Magellanic Clouds. I. New spectral classifications of OB types in the LMC. CONTI P.S., GARMANY C.D. and MASSEY P.
1992A&AS...92..729S 14       D               321 42 Spectral types and UBV magnitudes of stars in the 30 Doradus complex. SCHILD H. and TESTOR G.
1993A&A...278...11H 74 12 HDE 269828 : a reddened massive star cluster. HEYDARI-MALAYERI M., GREBEL E.K., MELNICK J., et al.
1993A&A...280..426T 97 14 The OB association LH 90 in the LMC : its age structure and Wolf-Rayet stars. TESTOR G., SCHILD H. and LORTET M.C.
2000AJ....119.2214M viz 653 146 The progenitor masses of Wolf-Rayet stars and luminous blue variables determined from cluster turnoffs. I. Results from 19 OB associations in the Magellanic clouds. MASSEY P., WATERHOUSE E. and DEGIOIA-EASTWOOD K.
2004ApJ...602..257B 27 41 Thermal and nonthermal x-rays from the Large Magellanic Cloud superbubble 30 Doradus C. BAMBA A., UENO M., NAKAJIMA H., et al.
2004ApJ...617.1316P 62 28 Effects of metallicity on the rotational velocities of massive stars. PENNY L.R., SPRAGUE A.J., SEAGO G., et al.
2009ApJ...700..844P viz 15       D               1 319 28 A FUSE survey of the rotation rates of very massive stars in the Small and Large Magellanic Clouds. PENNY L.R. and GIES D.R.
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.
2010AJ....139.1283W 128       D     X         4 39 26 The Onfp class in the Magellanic clouds. WALBORN N.R., HOWARTH I.D., EVANS C.J., et al.
2012ApJ...748...96M viz 15       D               2 64 36 Photometric and spectroscopic studies of massive binaries in the Large Magellanic Cloud. I. Introduction and orbits for two detached systems: evidence for a mass discrepancy? MASSEY P., MORRELL N.I., NEUGENT K.F., et al.
2013AcA....63..159U viz 15       D               1 768 16 Variable stars from the OGLE-III Shallow Survey in the Large Magellanic Cloud. ULACZYK K., SZYMANSKI M.K., UDALSKI A., et al.
2018A&A...615A..49C viz 16       D               1 224763 54 Characterising open clusters in the solar neighbourhood with the Tycho-Gaia Astrometric Solution. CANTAT-GAUDIN T., VALLENARI A., SORDO R., et al.
2023A&A...674A..16M viz 17       D               1 2184478 19 Gaia Data Release 3 The first Gaia catalogue of eclipsing-binary candidates. MOWLAVI N., HOLL B., LECOEUR-TAIBI I., et al.
2023A&A...674A..34G viz 17       D               1 307215 85 Gaia Data Release 3 Stellar multiplicity, a teaser for the hidden treasure. GAIA COLLABORATION, ARENOU F., BABUSIAUX C., 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.
2024MNRAS.530.4219C 108       D     X         3 48 ~ Thermal X-ray emission in the western half of the LMC superbubble 30 Dor C. CHI Y.-H., CHEN H.-X., CHEN Y., 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.
2025ApJ...994..159M 19       D               1 306 ~ On the Spatial Distribution of Luminous Blue Variables, B[e] Supergiants, and Wolf-Rayet Stars in the Large Magellanic Cloud. MARTIN J.C., HUMPHREYS R.M. and DAVIDSON K.

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