BI 272 , the SIMBAD biblio

BI 272 , the SIMBAD biblio (23 results) C.D.S. - SIMBAD4 rel 1.8 - 2023.03.27CEST00:33:30


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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.
1986AJ.....92...48C 244 111 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.
1999MNRAS.306..279S viz 879 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.
2001ApJ...550..724L 61 85 Ultraviolet line spectra of metal-poor star-forming galaxies. LEITHERER C., LEAO J.R.S., HECKMAN T.M., et al.
2002ApJ...566..857T 71 156 A far ultraviolet spectroscopic explorer survey of interstellar molecular hydrogen in the Small and Large Magellanic Clouds. TUMLINSON J., SHULL J.M., RACHFORD B.L., et al.
2002ApJS..139...81D 108 43 An atlas of far ultraviolet spectroscopic explorer sight lines toward the Magellanic clouds. DANFORTH C.W., HOWK J.C., FULLERTON A.W., et al.
2003ApJ...586..996M 31 87 Constraints the ionization balance of hot-star winds from FUSE observations of O stars in the Large Magellanic Cloud. MASSA D., FULLERTON A.W., SONNEBORN G., et al.
2003ApJ...589..526L 68 7 Far Spectroscopic Explorer snapshot survey of O VI variability in the winds of 66 OB-type stars. LEHNER N., FULLERTON A.W., MASSA D., et al.
2003ApJS..144...21R viz 15       D               261 45 Synthetic high-resolution line spectra of star-forming galaxies below 1200 Å. ROBERT C., PELLERIN A., ALOISI A., et al.
2006ApJ...646..205D 21 8 Possible detection of O VI from the Large Magellanic Cloud superbubble N70. DANFORTH C.W. and BLAIR W.P.
2007MNRAS.377..687L 128       D     X   F     3 44 30 Highly ionized plasma in the Large Magellanic Cloud: evidence for outflows and a possible galactic wind. LEHNER N. and HOWK J.C.
2009PASP..121..634B viz 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...700..844P viz 15       D               2 319 28 A FUSE survey of the rotation rates of very massive stars in the Small and Large Magellanic Clouds. PENNY L.R. and GIES D.R.
2009ApJ...702..940L viz 53       D     X         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 viz 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 viz 15       D               3 463 26 Interstellar Ti II in the Milky way and Magellanic clouds. WELTY D.E. and CROWTHER P.A.
2012ApJ...745..173W viz 16       D               2 307 47 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.
2012ApJS..199....8G viz 16       D               3 3036 46 A compilation of interstellar column densities. GUDENNAVAR S.B., BUBBLY S.G., PREETHI K., et al.
2015ApJ...811...78T viz 16       D               1 90 21 Elemental depletions in the Magellanic Clouds and the evolution of depletions with metallicity. TCHERNYSHYOV K., MEIXNER M., SEALE J., et al.
2016MNRAS.458..624C 16       D               1 123 55 The R136 star cluster dissected with Hubble Space Telescope/STIS. I. Far-ultraviolet spectroscopic census and the origin of He II λ1640 in young star clusters. CROWTHER P.A., CABALLERO-NIEVES S.M., BOSTROEM K.A., et al.
2017MNRAS.470.3765M viz 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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2023.03.27-00:33:30

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