SV* HV 2275 , the SIMBAD biblio

SV* HV 2275 , the SIMBAD biblio (22 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.15CEST17:05:01


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Title First 3 Authors
1978A&AS...32...83B 104 34 Photometry of Cepheid variables in the Large Magellanic Cloud. BUTLER C.J.
1988MNRAS.232...53R 150 58 A survey for red variables in the LMC. II. REID N., GLASS I.S. and CATCHPOLE R.M.
1995MNRAS.275..331R 330 23 Long-period variables in the Large Magellanic Cloud. IV. A compendium of northern variables. REID I.N., HUGHES S.M.G. and GLASS I.S.
2008AJ....136...18W viz 15       D               1 1226 186 Spitzer SAGE survey of the Large Magellanic Cloud. III. Star formation and ∼1000 new candidate young stellar objects. WHITNEY B.A., SEWILO M., INDEBETOUW R., et al.
2008AJ....136.1242F viz 15       D               1 47759 44 The properties of long-period variables in the Large Magellanic Cloud from MACHO. FRASER O.J., HAWLEY S.L. and COOK K.H.
2009MNRAS.397..933M viz 52       D     X         2 202 47 Period-luminosity relations for type II Cepheids and their application. MATSUNAGA N., FEAST M.W. and MENZIES J.W.
2008AcA....58..293S viz 15       D               1 292 159 The Optical Gravitational Lensing Experiment. The OGLE-III catalog of variable stars. II. Type II Cepheids and anomalous Cepheids in the Large Magellanic Cloud. SOSZYNSKI I., UDALSKI A., SZYMANSKI M.K., et al.
2011A&A...530A..90V viz 15       D               1 1414 46 The optically bright post-AGB population of the LMC. VAN AARLE E., VAN WINCKEL H., LLOYD EVANS T., et al.
2011A&A...536A..60S viz 15       D               1 43415 15 Long period variables in the Large Magellanic Cloud from the EROS-2 survey. SPANO M., MOWLAVI N., EYER L., et al.
2015MNRAS.446.3034R viz 16       D               2 142 37 The VMC Survey - XIII. Type II Cepheids in the Large Magellanic Cloud. RIPEPI V., MORETTI M.I., MARCONI M., et al.
2015MNRAS.453..133G viz 16       D               1 236 57 The WISE view of RV Tauri stars. GEZER I., VAN WINCKEL H., BOZKURT Z., et al.
2015MNRAS.454.1468K viz 16       D               1 2116 79 Optically visible post-AGB stars, post-RGB stars and young stellar objects in the Large Magellanic Cloud. KAMATH D., WOOD P.R. and VAN WINCKEL H.
2017A&A...603A..70G viz 16       D               2 344 10 Luminosities and infrared excess in Type II and anomalous Cepheids in the Large and Small Magellanic Clouds. GROENEWEGEN M.A.T. and JURKOVIC M.I.
2017A&A...604A..29G viz 16       D               1 353 11 The period-luminosity and period-radius relations of Type II and anomalous Cepheids in the Large and Small Magellanic Clouds. GROENEWEGEN M.A.T. and JURKOVIC M.I.
2018A&A...618A..21M 297       D     X         8 74 7 The evolutionary nature of RV Tauri stars in the SMC and LMC. MANICK R., VAN WINCKEL H., KAMATH D., et al.
2018AcA....68...89S viz 96       D     X         3 357 16 The OGLE Collection of Variable Stars. Type II Cepheids in the Magellanic System. SOSZYNSKI I., UDALSKI A., SZYMANSKI M.K., et al.
2019A&A...622A..60C viz 16       D               1 150347 194 Gaia Data Release 2. Specific characterisation and validation of all-sky Cepheids and RR Lyrae stars. CLEMENTINI G., RIPEPI V., MOLINARO R., et al.
2019MNRAS.486.3524K 1316       D     X C       32 11 ~ Extrinsically metal-poor stars: photospheric chemical depletion in post-AGB/post-RGB stars in the Large Magellanic Cloud. KAMATH D. and VAN WINCKEL H.
2020A&A...636A..48G viz 16       D               1 970 ~ The VMC Survey. XXXVII. Pulsation periods of dust-enshrouded AGB stars in the Magellanic Clouds. GROENEWEGEN M.A.T., NANNI A., CIONI M.-R.L., et al.
2024MNRAS.530..761M 18       D               1 48 ~ The first measurements of carbon isotopic ratios in post-RGB stars: SZ Mon and DF Cyg. MOHORIAN M., KAMATH D., MENON M., et al.
2024A&A...685A..41S viz 18       D               1 371 ~ The VMC survey L. Type II Cepheids in the Magellanic Clouds: Period-luminosity relations in the near-infrared bands. SICIGNANO T., RIPEPI V., MARCONI M., et al.
2025A&A...703A.294M viz 140           X C       2 14 ~ Understanding post-red giant branch binaries through stable mass transfer. MOLTZER C.A.S., POLS O.R., VAN WINCKEL H., et al.

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