CPD-69 445 , the SIMBAD biblio

CPD-69 445 , the SIMBAD biblio (21 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.14CEST09:56:17


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Title First 3 Authors
1970CoTol..89....1S viz 13       D               1286 ~ A deep objective-prism survey for Large Magellanic Cloud members. SANDULEAK N.
1991PASP..103.1123F 88 58 A spectroscopic survey of subgiants in the Large Magellanic Cloud. FITZPATRICK E.L.
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.
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...749..177N viz 15       D               1 1994 81 Yellow and red supergiants in the Large Magellanic Cloud. NEUGENT K.F., MASSEY P., SKIFF B., et al.
2015MNRAS.451.4346S viz 55       D     X         2 177 7 Large- and small-scale structure of the intermediate- and high-velocity clouds towards the LMC and SMC. SMOKER J.V., FOX A.J. and KEENAN F.P.
2015A&A...584A...5E viz 16       D               1 275 9 2dF-AAOmega spectroscopy of massive stars in the Magellanic Clouds. The north-eastern region of the Large Magellanic Cloud. EVANS C.J., VAN LOON J.T., HAINICH R., et al.
2017AJ....154..102U viz 16       D               7 104 13 LMC blue supergiant stars and the calibration of the Flux-weighted Gravity-Luminosity Relationship. URBANEJA M.A., KUDRITZKI R.-P., GIEREN W., 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.
2019ApJ...872L...9P viz 16       D               2 157 56 Diverse variability of O and B stars revealed from 2-minute cadence light curves in sectors 1 and 2 of the TESS mission: selection of an asteroseismic sample. PEDERSEN M.G., CHOWDHURY S., JOHNSTON C., et al.
2019MNRAS.485.3457B viz 16       D               1 194 44 Rotational modulation in TESS B stars. BALONA L.A., HANDLER G., CHOWDHURY S., et al.
2020ApJ...889..179G 16       D               1 98 38 Empirical calibration of the reddening maps in the Magellanic Clouds. GORSKI M., ZGIRSKI B., PIETRZYNSKI G., 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.
2022ApJ...924..117B viz 17       D               1 161 4 Rotation signature of TESS B-type stars. A comprehensive analysis. BARRAZA L.F., GOMES R.L., MESSIAS Y.S., 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.
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...676A..85S 17       D               2 127 ~ The ESO UVES/FEROS Large Programs of TESS OB pulsators I. Global stellar parameters from high-resolution spectroscopy. SEREBRIAKOVA N., TKACHENKO A., GEBRUERS S., et al.
2024ApJ...963L..42M 18       D               1 65 ~ Evidence for Evolved Stellar Binary Mergers in Observed B-type Blue Supergiants. MENON A., ERCOLINO A., URBANEJA M.A., et al.
2024A&A...692A.245S viz 18       D               1 192 ~ The ESO UVES/FEROS Large Programs of TESS OB pulsators II. The physical origin of macroturbulence. SEREBRIAKOVA N., TKACHENKO A. and AERTS C.

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