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| BI 259 , the SIMBAD biblio (10 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.15CEST16:16:59 |
| 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 |
|---|---|---|---|---|---|---|---|---|---|
| 1975A&AS...21..109B | 13 | D | 274 | 74 | Recherches dans le Grand Nuage de Magellan. I. Un catalogue de 272 etoiles O-B2 nouvelles. | BRUNET J.P., IMBERT M., MARTIN N., et al. | |||
| 2000A&A...353..655K | 34 | 49 | Chemical abundances from Magellanic cloud B stars. | KORN A.J., BECKER S.R., GUMMERSBACH C.A., et al. | |||||
|
2002ApJS..141...81M |
1417 | 322 | A UBVR CCD survey of the Magellanic clouds. | MASSEY P. | |||||
|
2011A&A...530A.108E |
15 | D | 1 | 950 | 254 | The VLT-FLAMES Tarantula Survey. I. Introduction and observational overview. | EVANS C.J., TAYLOR W.D., HENAULT-BRUNET V., et al. | ||
|
2013A&A...550A.107S |
15 | D | 1 | 347 | 382 | The VLT-FLAMES Tarantula Survey. VIII. Multiplicity properties of the O-type star population. | SANA H., DE KOTER A., DE MINK S.E., et al. | ||
|
2013A&A...550A.108V |
15 | D | 1 | 864 | 59 | The VLT-FLAMES Tarantula Survey. IX. The interstellar medium seen through diffuse interstellar bands and neutral sodium. | VAN LOON J.T., BAILEY M., TATTON B.L., et al. | ||
|
2014A&A...564A..40W |
15 | D | 1 | 377 | 85 | The VLT-FLAMES Tarantula Survey. XIV. The O-type stellar content of 30 Doradus. | WALBORN N.R., SANA H., SIMON-DIAZ S., et al. | ||
|
2017A&A...598A..84A |
135 | D | X C | 3 | 112 | 96 | The Tarantula Massive Binary Monitoring. I. Observational campaign and OB-type spectroscopic binaries. | ALMEIDA L.A., SANA H., TAYLOR W., et al. | |
| 2020A&A...634A.118M | 346 | D | S X C | 7 | 61 | 41 | The Tarantula Massive Binary Monitoring. III. Atmosphere analysis of double-lined spectroscopic systems. | MAHY L., SANA H., ABDUL-MASIH M., et al. | |
|
2023ApJ...952...64L |
17 | D | 1 | 2632 | ~ | Massive Hypervelocity Runaway Stars in the Large Magellanic Cloud. | LIN Z., XU Y., HAO C., et al. |