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BI 128 , the SIMBAD biblio (10 results) | C.D.S. - SIMBAD4 rel 1.8 - 2023.03.24CET16:44:23 |
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 | 14 | 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. | |||
1982A&AS...50....7I | 247 | 28 | Photoelektrische UBV-Photometrie in der Grossen Magellanschen Wolke. | ISSERSTEDT J. | |||||
1995ApJ...438..188M | 308 | 347 | Massive stars in the field and associations of the Magellanic Clouds : the upper mass limit, the initial mass function and a critical test of main-sequence stellar evolutionary theory. | MASSEY P., LANG C.C., DE GIOIA-EASTWOOD K., et al. | |||||
2009PASP..121..634B ![]() |
15 | D | 1 | 288 | 10 | The Far Ultraviolet Spectroscopic Explorer legacy in the Magellanic Clouds: an online stellar sight line atlas. | BLAIR W.P., OLIVEIRA C., LAMASSA S., et al. | ||
2009ApJ...702..940L ![]() |
15 | D | 2 | 153 | 16 | Properties and origin of the high-velocity gas toward the Large Magellanic Cloud. | LEHNER N., STAVELEY-SMITH L. and HOWK J.C. | ||
2009AJ....138.1003B ![]() |
15 | D | 1 | 1760 | 67 | Spitzer SAGE infrared photometry of massive stars in the Large Magellanic Cloud. | BONANOS A.Z., MASSA D.L., SEWILO M., et al. | ||
2010MNRAS.404.1321W ![]() |
15 | D | 3 | 463 | 26 | Interstellar Ti II in the Milky way and Magellanic clouds. | WELTY D.E. and CROWTHER P.A. | ||
2012ApJS..199....8G ![]() |
16 | D | 3 | 3036 | 46 | A compilation of interstellar column densities. | GUDENNAVAR S.B., BUBBLY S.G., PREETHI K., et al. | ||
2015MNRAS.451.4346S ![]() |
16 | D | 2 | 177 | 7 | Large- and small-scale structure of the intermediate- and high-velocity clouds towards the LMC and SMC. | SMOKER J.V., FOX A.J. and KEENAN F.P. | ||
2017MNRAS.470.3765M ![]() |
16 | D | 1 | 109 | 2 | Mass-loss rates from mid-infrared excesses in LMC and SMC O stars. | MASSA D., FULLERTON A.W. and PRINJA R.K. |
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