BAT99 80 , the SIMBAD biblio

BAT99 80 , the SIMBAD biblio (23 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.14CEST17:29:05

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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
1990A&A...240..299T 13 14 New Wolf-Rayet and extreme Of stars near the 30 Doradus nebula. TESTOR G. and SCHILD H.
1991IAUS..143..513L 15 7 Nomenclature problems. LORTET M.-C.
1992A&AS...92..729S 14       D               321 42 Spectral types and UBV magnitudes of stars in the 30 Doradus complex. SCHILD H. and TESTOR G.
1993A&A...278...11H 74 12 HDE 269828 : a reddened massive star cluster. HEYDARI-MALAYERI M., GREBEL E.K., MELNICK J., et al.
1993A&A...280..426T 97 14 The OB association LH 90 in the LMC : its age structure and Wolf-Rayet stars. TESTOR G., SCHILD H. and LORTET M.C.
1994ApJS...93..455D 203 48 An atlas of the interstellar environment of Wolf-Rayet stars in the Magellanic Clouds. DOPITA M.A., BELL J.F., CHU Y.-H., et al.
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.
1999AJ....118.1684W viz 40 54 HST/FOS spatially resolved spectral classification of compact OB groups in the Large Magellanic Cloud. WALBORN N.R., DRISSEN L., PARKER J.W., et al.
2000AJ....119.2214M viz 653 146 The progenitor masses of Wolf-Rayet stars and luminous blue variables determined from cluster turnoffs. I. Results from 19 OB associations in the Magellanic clouds. MASSEY P., WATERHOUSE E. and DEGIOIA-EASTWOOD K.
2002ApJS..141...81M viz 1417 322 A UBVR CCD survey of the Magellanic clouds. MASSEY P.
2008ApJS..177..216G 89       D       C       8 78 18 An X-ray survey of Wolf-Rayet stars in the Magellanic Clouds. I. The chandra ACIS data set. GUERRERO M.A. and CHU Y.-H.
2008ApJS..177..238G 238       D     X         7 143 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 313       D     X   F     8 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.
2011MNRAS.416.1311C 76             C       2 67 84 Spectral classification of O2–3.5 If*/WN5–7 stars. CROWTHER P.A. and WALBORN N.R.
2013A&A...555A.141H viz 15       D               1 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.
2018ApJ...863..181N viz 177       D     X         5 190 39 A modern search for Wolf-Rayet Stars in the Magellanic Clouds. IV. A final census. NEUGENT K.F., MASSEY P. and MORRELL N.
2019A&A...627A.151S 219       D   O X C       5 76 55 The Wolf-Rayet binaries of the nitrogen sequence in the Large Magellanic Cloud. Spectroscopy, orbital analysis, formation, and evolution. SHENAR T., SABLOWSKI D.P., HAINICH R., et al.
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.
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.
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.
2024MNRAS.530.4219C 63       D     X         2 48 ~ Thermal X-ray emission in the western half of the LMC superbubble 30 Dor C. CHI Y.-H., CHEN H.-X., CHEN Y., et al.
2025ApJ...994..159M 19       D               2 306 ~ On the Spatial Distribution of Luminous Blue Variables, B[e] Supergiants, and Wolf-Rayet Stars in the Large Magellanic Cloud. MARTIN J.C., HUMPHREYS R.M. and DAVIDSON K.

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