Cl* NGC 1866 WE 2 , the SIMBAD biblio

Cl* NGC 1866 WE 2 , the SIMBAD biblio (11 results) C.D.S. - SIMBAD4 rel 1.8 - 2024.04.24CEST01:20:49


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Title First 3 Authors
1991AJ....101..490W 53 55 The variable stars of NGC 1866. WELCH D.L., MATEO M., COTE P., et al.
1993AJ....105.1813W 1 37 231 Robust variable star detection techniques suitable for automated searches: new results for NGC 1866. WELCH D.L. and STETSON P.B.
2004AJ....128.1597B 23 16 Pulsational evidence for mass loss in NGC 1866 cepheids. BROCATO E., CAPUTO F., CASTELLANI V., et al.
2007A&A...462..599T viz 34 11 Infrared photometry of Cepheids in the LMC clusters NGC 1866 and NGC 2031. TESTA V., MARCONI M., MUSELLA I., et al.
2012ApJ...748...69M 1021       D     X C       26 18 15 CORS baade-wesselink distance to the LMC NGC 1866 blue populous cluster. MOLINARO R., RIPEPI V., MARCONI M., et al.
2013A&A...550A..70G viz 39           X         1 201 45 Baade-Wesselink distances to Galactic and Magellanic Cloud Cepheids and the effect of metallicity. GROENEWEGEN M.A.T.
2013MNRAS.428.2185M 601       D S   X C       14 10 15 Theoretical fit of Cepheid light a radial velocity curves in the Large Magellanic Cloud cluster NGC 1866. MARCONI M., MOLINARO R., RIPEPI V., et al.
2014A&A...566A..37G viz 16       D               1 601 158 On the fine structure of the Cepheid metallicity gradient in the Galactic thin disk. GENOVALI K., LEMASLE B., BONO G., et al.
2016MNRAS.457.3084M 16       D               1 36 5 The Cepheids of NGC 1866: a precise benchmark for the extragalactic distance scale and stellar evolution from modern UBVI photometry. MUSELLA I., MARCONI M., STETSON P.B., et al.
2017A&A...608A..85L 41           X         1 46 8 Detailed chemical composition of classical Cepheids in the LMC cluster NGC 1866 and in the field of the SMC. LEMASLE B., GROENEWEGEN M.A.T., GREBEL E.K., et al.
2019A&A...631A.128C 18       D               2 11 18 Multiple stellar populations in NGC 1866. New clues from Cepheids and colour-magnitude diagram. COSTA G., GIRARDI L., BRESSAN A., et al.

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