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| BI 192 , the SIMBAD biblio (10 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.15CEST13:39:33 |
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More on score
| 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. | |||
| 1986AJ.....92...48C | 244 | 119 | Studies of massive stars in the Magellanic Clouds. I. New spectral classifications of OB types in the LMC. | CONTI P.S., GARMANY C.D. and MASSEY P. | |||||
| 1998MNRAS.300..828P | 82 | 40 | HST UV measurements of wind structure and velocities in Local Group OB stars. | PRINJA R.K. and CROWTHER P.A. | |||||
| 2001ApJ...550..724L | 61 | 99 | Ultraviolet line spectra of metal-poor star-forming galaxies. | LEITHERER C., LEAO J.R.S., HECKMAN T.M., et al. | |||||
2002ApJS..141...81M 
|
1417 | 322 | A UBVR CCD survey of the Magellanic clouds. | MASSEY P. | |||||
| 2009ApJ...692..618M | 315 | D | X C F | 7 | 38 | 33 | The physical properties and effective temperature scale of O-type stars as a function of metallicity. III. More results from the Magellanic clouds. | MASSEY P., ZANGARI A.M., MORRELL N.I., et al. | |
|
2009AJ....138.1003B
|
15 | D | 1 | 1760 | 163 | Spitzer SAGE infrared photometry of massive stars in the Large Magellanic Cloud. | BONANOS A.Z., MASSA D.L., SEWILO M., et al. | ||
|
2012ApJ...745..173W
|
15 | D | 1 | 307 | 56 | Interstellar H I and H2 in the Magellanic Clouds: an expanded sample based on ultraviolet absorption-line data. | WELTY D.E., XUE R. and WONG T. | ||
| 2022AJ....163...30L | 102 | D | X | 3 | 17 | ~ | The shellless supernova remnant B0532-67.5 in the Large Magellanic Cloud. | LI C.-J., CHU Y.-H., CHUANG C.-Y., 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. |
