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| SK -69 140 , the SIMBAD biblio (10 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.15CEST10:41:36 |
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| Bibcode/DOI | Score |
in Title|Abstract| Keywords |
in a table | in teXt, Caption, ... | Nb occurence | Nb objects in ref |
Citations (from ADS) |
Title | First 3 Authors |
|---|---|---|---|---|---|---|---|---|---|
1970CoTol..89....1S 
|
13 | D | 1286 | ~ | A deep objective-prism survey for Large Magellanic Cloud members. | SANDULEAK N. | |||
| 1982A&AS...50....7I | 247 | 28 | Photoelektrische UBV-Photometrie in der Grossen Magellanschen Wolke. | ISSERSTEDT J. | |||||
|
1999MNRAS.306..279S
|
878 | 13 | UBV photometry of Galactic foreground and LMC member stars - III. LMC member stars - a new data base. | SCHMIDT-KALER T., GOCHERMANN J., OESTREICHER M.O., et al. | |||||
|
2002ApJS..141...81M
|
1417 | 322 | A UBVR CCD survey of the Magellanic clouds. | MASSEY P. | |||||
|
2023A&A...675A.154V
|
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.52711422P | 287 | D | S C F | 6 | 43 | ~ | Optically thick structure in early B-type supergiant stellar winds at low metallicities. | PARSONS T.N., PRINJA R.K., BERNINI-PERON M., et al. | |
| 2024A&A...688A.105H | 18 | D | 1 | 171 | ~ | X-Shooting ULLYSES: Massive stars at low metallicity III. Terminal wind speeds of ULLYSES massive stars. | HAWCROFT C., SANA H., MAHY L., et al. | ||
| 2024ApJ...974...22Z | 18 | D | 1 | 120 | ~ | Braving the Storm: Quantifying Disk-wide Ionized Outflows in the Large Magellanic Cloud with ULLYSES. | ZHENG Y., TCHERNYSHYOV K., OLSEN K., et al. | ||
| 2024A&A...692A..91V | 18 | D | 4 | 20 | ~ | X-Shooting ULLYSES: Massive Stars at low metallicity IX. Empirical constraints on mass-loss rates and clumping parameters for OB supergiants in the Large Magellanic Cloud. | VERHAMME O., SUNDQVIST J., DE KOTER A., et al. | ||
|
2025A&A...695A.198B
|
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. |
