SK 179 , the SIMBAD biblio

SK 179 , the SIMBAD biblio (12 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.14CEST20:19:09


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Title First 3 Authors
1969AJ.....74..877S 48 71 Proven and probable members in the Wing of the Small Magellanic Cloud. SANDULEAK N.
1976A&AS...24..357S 315 50 Starlight polarization in the Magellanic Cloud regions. SCHMIDT T.
1978A&AS...33..193I 104 25 Lichtelektrische Photometrie in der Kleinen Magellanschen Wolke. ISSERSTEDT J.
1987A&AS...69..421A 297 14 Small Magellanic Cloud : H gamma-line equivalent widths and luminosity classes of the brightest blue star members. AZZOPARDI M.
2002ApJS..141...81M viz 1417 322 A UBVR CCD survey of the Magellanic clouds. MASSEY P.
2014ASPC..485..223B viz 15       D               1 465820 45 The JMMC stellar diameters catalog v2 (JSDC): a new release based on SearchCal improvements BOURGES L., LAFRASSE S., MELLA G., et al.
2019A&A...629A..91Y viz 16       D               1 1374 29 Evolved massive stars at low-metallicity. I. A source catalog for the Small Magellanic Cloud. YANG M., BONANOS A.Z., JIANG B.-W., et al.
2019MNRAS.490.3158C viz 16       D               1 465839 28 A catalogue of stellar diameters and fluxes for mid-infrared interferometry. CRUZALEBES P., PETROV R.G., ROBBE-DUBOIS S., 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...692A..89B 376       D     X C       8 33 ~ X-Shooting ULLYSES: Massive stars at low metallicity VII. Stellar and wind properties of B supergiants in the Small Magellanic Cloud. BERNINI-PERON M., SANDER A.A.C., RAMACHANDRAN V., et al.
2025A&A...695A.198B viz 65       D     X         2 247 ~ 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.
2025A&A...697A.114P viz 19       D               1 198 ~ New empirical mass-loss recipe for UV radiation line-driven winds of hot stars across various metallicities. PAULI D., OSKINOVA L.M., HAMANN W.-R., et al.

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