[MA93] 1380 , the SIMBAD biblio

[MA93] 1380 , the SIMBAD biblio (10 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.16CEST21:50:05


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Title First 3 Authors
1993A&AS..102..451M viz 14       D               1 1968 135 A new catalogue of H-alpha emission-line stars and small nebulae in the Small Magellanic Cloud. MEYSSONNIER N. and AZZOPARDI M.
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.
2003A&A...401..873W viz 526 26 The Small Magellanic Cloud in the far infrared. I. ISO's 170 µm map and revisit of the IRAS 12-100 µm data. WILKE K., STICKEL M., HAAS M., et al.
2004AJ....127.1632O viz 1516 61 Massive field stars and the stellar clustering law. OEY M.S., KING N.L. and PARKER J.W.
2006ApJ...652..458W viz 15       D               564 58 The role of evolutionary age and metallicity in the formation of classical Be circumstellar disks. I. New candidate Be stars in the LMC, SMC, and Milky Way. WISNIEWSKI J.P. and BJORKMAN K.S.
2007ApJ...671.2040W viz 15       D               418 18 The role of evolutionary age and metallicity in the formation of classical Be circumstellar disks. II. Assessing the evolutionary nature of candidate disk systems. WISNIEWSKI J.P., BJORKMAN K.S., MAGALHAES A.M., et al.
2017NewA...56...28P viz 16       D               1 419 1 NIR properties of Be stars in star clusters in the Magellanic Clouds. PAUL K.T., ANNAPURNI S., BLESSON M., et al.
2022ApJ...936..112D viz 17       D               1 1353 3 Classical OBe Stars as Post-supernova Runaways: Confirming Binary Origins. DALLAS M.M., OEY M.S. and CASTRO N.
2024A&A...690A.289S viz 18       D               1 941 ~ Binarity at LOw Metallicity (BLOeM) A spectroscopic VLT monitoring survey of massive stars in the SMC. SHENAR T., BODENSTEINER J., SANA H., et al.
2025A&A...698A..38B viz 19       D               1 94 ~ Binarity at LOw Metallicity (BLOeM) Multiplicity properties of Oe and Be stars. BODENSTEINER J., SHENAR T., SANA H., et al.

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