PGMW 3168 , the SIMBAD biblio

PGMW 3168 , the SIMBAD biblio (22 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.16CEST16:22:07


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Title First 3 Authors
1992AJ....103.1205P viz 1237 159 The stellar content of LH 9 and 10 (N11) in the LMC: a case for sequential star formation. PARKER J.W., GARMANY C.D., MASSEY P., et al.
1996A&A...308..588R 29 47 Formation of the nebular complex N11 in the Large Magellanic Cloud. ROSADO M., LAVAL A., LE COARER E., et al.
2001AJ....122..921N 38 37 Interstellar bubbles in two young H II regions. NAZE Y., CHU Y.-H., POINTS S.D., et al.
2003AJ....125.1940B viz 216 18 Active star formation in the N11B nebula in the Large Magellanic Cloud: a sequential star formation scenario confirmed. BARBA R.H., RUBIO M., ROTH M.R., et al.
2006A&A...456..623E viz 516 176 The VLT-FLAMES survey of massive stars: observations centered on the Magellanic Cloud clusters NGC330, NGC346, NGC2004, and the N11 region. EVANS C.J., LENNON D.J., SMARTT S.J., et al.
2007A&A...465.1003M 15       D               1 134 135 The VLT-FLAMES survey of massive stars: wind properties and evolution of hot massive stars in the Large Magellanic Cloud. MOKIEM M.R., DE KOTER A., EVANS C.J., et al.
2007A&A...473..603M 15       D               1 123 294 The empirical metallicity dependence of the mass-loss rate of O- and early B-type stars. MOKIEM M.R., DE KOTER A., VINK J.S., et al.
2008A&A...479..541H viz 15       D               407 164 The VLT-FLAMES survey of massive stars: atmospheric parameters and rotational velocity distributions for B-type stars in the Magellanic Clouds. HUNTER I., LENNON D.J., DUFTON P.L., et al.
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 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 viz 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.
2010ApJ...718L.141P viz 15       D               2 56 7 Far-ultraviolet diffuse emission from the Large Magellanic Cloud. PRADHAN A.C., PATHAK A. and MURTHY J.
2012A&A...537A..79R 474       D     X C F     11 36 77 Nitrogen line spectroscopy of O-stars. II. Surface nitrogen abundances for O-stars in the Large Magellanic Cloud. RIVERO GONZALEZ J.G., PULS J., NAJARRO F., et al.
2012A&A...548A..91L 15       D               1 44 51 Physical conditions in the gas phases of the giant H II region LMC-N11 unveiled by Herschel. I. Diffuse [C II] and [O III] emission in LMC-N11B. LEBOUTEILLER V., CORMIER D., MADDEN S.C., et al.
2016A&A...591A.118S viz 16       D               1 31408 141 The PASTEL catalogue: 2016 version. SOUBIRAN C., LE CAMPION J.-F., BROUILLET N., et al.
2023ApJ...952...64L viz 17       D               1 2632 ~ Massive Hypervelocity Runaway Stars in the Large Magellanic Cloud. LIN Z., XU Y., HAO C., et al.
2023A&A...675A.154V viz 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.
2024A&A...689A..31M 18       D               3 155 ~ X-Shooting ULLYSES: Massive stars at low metallicity V. Effect of metallicity on surface abundances of O stars. MARTINS F., BOURET J.-C., HILLIER D.J., et al.
2025A&A...695A.197G 392       D     X         9 36 ~ X-Shooting ULLYSES: Massive stars at low metallicity X. Physical parameters and feedback of massive stars in the LMC N11 B star-forming region. GOMEZ-GONZALEZ V.M.A., OSKINOVA L.M., HAMANN W.-R., et al.
2025A&A...695A.198B viz 112       D     X         3 247 ~ 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.
2025A&A...697A.114P viz 19       D               1 198 ~ New empirical mass-loss recipe for UV radiation line-driven winds of hot stars across various metallicities. PAULI D., OSKINOVA L.M., HAMANN W.-R., et al.

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