LHA 120-S 142 , the SIMBAD biblio

LHA 120-S 142 , the SIMBAD biblio (38 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.17CEST06:52:18


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Title First 3 Authors
1956ApJS....2..315H 911 846 Catalogues of H-alpha emission stars and nebulae in the Magellanic Clouds. HENIZE K.G.
1963IrAJ....6..127L 363 22 Second list of emission-line objects in the Large Magellanic Cloud. LINDSAY E.M.
1970CoTol..89....1S viz 13       D               1286 ~ A deep objective-prism survey for Large Magellanic Cloud members. SANDULEAK N.
1974A&AS...18...47B 627 74 H alpha emission-line stars in the Large Magellanic Cloud. I. A new deep survey. BOHANNAN B. and EPPS H.W.
1975A&A....41..175I 30 58 Interstellar reddening in the Large Magellanic Cloud. ISSERSTEDT J.
1978A&AS...33..115F 76 12 Objets a emission dans le Grand Nuage de Magellan. FEHRENBACH C., DUFLOT M. and ACKER A.
1988BICDS..35..145L 80 3 A provisory catalogue of S-Dor candidate stars in the Magellanic Clouds. LORTET M.C.
1989PASP..101..520B 1 12 88 The Ofpe/WN9 class in the Large Magellanic Cloud. BOHANNAN B. and WALBORN N.R.
1995A&A...302..409G 60 55 B[e] phenomenon extending to lower luminosities in the Magellanic Clouds. GUMMERSBACH C.A., ZICKGRAF F.-J. and WOLF B.
1997A&A...318..543C 20 12 B 517 - Another very late WNL star in M 33. CROWTHER P.A., SZEIFERT T., STAHL O., et al.
1997A&A...320..500C 46 142 Fundamental parameters of Wolf-Rayet stars. VI. Large Magellanic Cloud WNL stars. CROWTHER P.A. and SMITH L.J.
1999A&AS..137..117B 225 155 The fourth catalogue of Population I Wolf-Rayet stars in the Large Magellanic Cloud. BREYSACHER J., AZZOPARDI M. and TESTOR G.
2002AcA....52...81N 167 25 Kinematical structure of Wolf-Rayet winds. I. Terminal wind velocity. NIEDZIELSKI A. and SKORZYNSKI W.
2004ApJ...601..228B 19 19 The Ofpe/WN9 stars in M33. BIANCHI L., BOHLIN R. and MASSEY P.
2004AcA....54..405N 117 3 Kinematical structure of Wolf-Rayet winds. II. Internal velocity scatter in WN stars. NIEDZIELSKI A., NUGIS T. and SKORZYNSKI W.
2005A&A...437..217F 7 20 Crowded field 3D spectroscopy of LBV candidates in M33. FABRIKA S., SHOLUKHOVA O., BECKER T., et al.
2008ApJS..177..238G 15       D               5 143 6 An X-ray survey of Wolf-Rayet stars in the Magellanic Clouds. II. The ROSAT PSPC and HRI data sets. GUERRERO M.A. and CHU Y.-H.
2008MNRAS.389..806S 89       D         F     7 61 27 A spectroscopic survey of WNL stars in the Large Magellanic Cloud: general properties and binary status. SCHNURR O., MOFFAT A.F.J., ST-LOUIS N., 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.
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.
2012ApJ...745..173W viz 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.
2012A&A...548A..16H viz 15       D               1 627 3 Improved astrometry for the Bohannan & Epps catalogue. HOWARTH I.D.
2013A&A...555A.141H viz 15       D               3 1714 3 Emission-line stars in the LMC: the Armagh survey and a metacatalogue. HOWARTH I.D.
2014A&A...565A..27H viz 132       D     X C       3 125 154 The Wolf-Rayet stars in the Large Magellanic Cloud. A comprehensive analysis of the WN class. HAINICH R., RUEHLING U., TODT H., et al.
2018A&A...615A..49C viz 16       D               1 224763 54 Characterising open clusters in the solar neighbourhood with the Tycho-Gaia Astrometric Solution. CANTAT-GAUDIN T., VALLENARI A., SORDO R., et al.
2018ApJ...863..181N viz 16       D               1 190 39 A modern search for Wolf-Rayet Stars in the Magellanic Clouds. IV. A final census. NEUGENT K.F., MASSEY P. and MORRELL N.
2020A&A...634A..79S 16       D   O           1 199 63 Why binary interaction does not necessarily dominate the formation of Wolf-Rayet stars at low metallicity. SHENAR T., GILKIS A., VINK J.S., et al.
2020ApJ...891..107R 16       D               2 39 ~ Massive stars in the SDSS-IV-APOGEE survey: Wolf-Rayet stars of the WN type. ROMAN-LOPES A., ROMAN-ZUNIGA C.G., BORISSOVA J., et al.
2021ApJS..252...21H viz 17       D               1 277 4 A multiwavelength Survey of Wolf-Rayet nebulae in the Large Magellanic Cloud. HUNG C.S., OU P.-S., CHU Y.-H., et al.
2021ApJ...913...32D viz 17       D               1 5182 ~ Photometric classifications of evolved massive stars: preparing for the era of webb and roman with machine learning. DORN-WALLENSTEIN T.Z., DAVENPORT J.R.A., HUPPENKOTHEN D., et al.
2022AJ....163..152S viz 17       D               1 583193 11 APOGEE Net: An Expanded Spectral Model of Both Low-mass and High-mass Stars. SPRAGUE D., CULHANE C., KOUNKEL M., et al.
2022ApJS..259...35A viz 17       D               1 611005 320 The Seventeenth Data Release of the Sloan Digital Sky Surveys: Complete Release of MaNGA, MaStar, and APOGEE-2 Data. ABDURRO'UF, ACCETTA K., AERTS C., et al.
2022A&A...667A..58P 17       D               1 137 5 A synthetic population of Wolf-Rayet stars in the LMC based on detailed single and binary star evolution models. PAULI D., LANGER N., AGUILERA-DENA D.R., et al.
2023MNRAS.521..585C 17       D               1 274 1 Line luminosities of Galactic and Magellanic Cloud Wolf-Rayet stars. CROWTHER P.A., RATE G. and BESTENLEHNER J.M.
2023A&A...672A.198S 17       D               1 34 1 Reverse Algols and hydrogen-rich Wolf-Rayet stars from very massive binaries. SEN K., LANGER N., PAULI D., 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.
2023MNRAS.525.2820K 17       D               1 95 ~ Cold diffuse interstellar medium of Magellanic Clouds: I. HD molecule and cosmic-ray ionization rate. KOSENKO D.N. and BALASHEV S.A.
2024ApJ...974..194S 18       D               1 46 ~ Formation of WNL Stars in the MW and LMC Based on the k - ω Model. SI J., LI Z. and LI Y.

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