SV* HV 12204 , the SIMBAD biblio

SV* HV 12204 , the SIMBAD biblio (33 results) C.D.S. - SIMBAD4 rel 1.8 - 2024.05.09CEST10:26:54

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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
1950AJ.....55..249S 30 ~ NGC 1866 and the Magellanic Cloud variables. SHAPLEY H. and McKIBBEN N.V.
1961ApJ...133..413H 50 98 Studies of the Large Magellanic Cloud. V. The young populous clusters. HODGE P.W.
1967ApJ...149...73A 21 70 The star cluster NGC 1866 and its Cepheids. ARP H. and THACKERAY A.D.
1987MNRAS.225..627W 18 54 CCD light curves for seven Cepheid variables in the LMC cluster NGC 1866. WALKER A.R.
1988A&A...190L..18S 16 22 The Cepheids of the young LMC cluster NGC 1866. STORM J., ANDERSEN J., BLECHA A., et al.
1991AJ....101..490W 53 55 The variable stars of NGC 1866. WELCH D.L., MATEO M., COTE P., et al.
1991AJ....101.1681C 9 18 Baade-Wesselink radii for NGC 1866 Cepheids. COTE P., WELCH D.L., MATEO M., et al.
1992PASP..104..824M 47 11 Tuning the Cepheid distance scale. MATEO M.
1993A&A...275..213F 3 3 On the difficulty of determining the color-term in the cepheid PLC relation. FOUQUE P. and GIEREN W.P.
1993ApJ...412..160B 28 19 The distance to the Large Magellanic Cloud : constraints from cepheids in Large Magellanic Cloud star clusters. BERTELLI G., BRESSAN A., CHIOSI C., et al.
1994ApJ...433L..73G 6 13 The distance to the Large Magellanic Cloud cluster NGC 1866 from its cepheid members. GIEREN W.P., RICHTLER T. and HILKER M.
1997MNRAS.290..353B 2 2 14 Cepheids in NGC 1866: a test for pulsational models. BONO G. and MARCONI M.
1998ApJ...496...17G 120 192 Cepheid period-radius and period-luminosity relations and the distance to the Large Magellanic Cloud. GIEREN W.P., FOUQUE P. and GOMEZ M.
2000ApJS..129..111G 10 9 Cepheid variables in the Large Magellanic Cloud cluster NGC 1866. I. New BVRI CCD photometry. GIEREN W.P., GOMEZ M., STORM J., et al.
2003A&A...410..887G 14 17 The distance to the LMC cluster NGC 1866 : clues from the cluster Cepheid population. GROENEWEGEN M.A.T. and SALARIS M.
2004AJ....128.1597B 23 16 Pulsational evidence for mass loss in NGC 1866 cepheids. BROCATO E., CAPUTO F., CASTELLANI V., et al.
2005A&A...440..487S viz         O           16 15 The near-IR surface brightness method applied to six Cepheids in the young LMC cluster NGC 1866. STORM J., GIEREN W.P., FOUQUE P., et al.
2005ApJ...627..224G 58 107 Direct distances to Cepheids in the Large Magellanic Cloud: evidence for a universal slope of the period-luminosity relation up to solar abundance. GIEREN W., STORM J., BARNES III T.G., et al.
2006MmSAI..77..261S 8 2 Distances to six Cepheids in the LMC cluster NGC 1866 from the near-IR surface-brightness method. STORM J., GIEREN W., FOUQUE P., et al.
2007A&A...476..863F 15       D               1 127 34 Classical Cepheid pulsation models. XI. Effects of convection and chemical composition on the period-luminosity and period-Wesenheit relations. FIORENTINO G., MARCONI M., MUSELLA I., et al.
2011A&A...534A..95S viz 16       D   O           1 43 108 Calibrating the Cepheid period-luminosity relation from the infrared surface brightness technique. II. The effect of metallicity and the distance to the LMC'. STORM J., GIEREN W., FOUQUE P., et al.
2012ApJ...748...69M 39           X         1 18 15 CORS baade-wesselink distance to the LMC NGC 1866 blue populous cluster. MOLINARO R., RIPEPI V., MARCONI M., et al.
2012MNRAS.426.3148S 93       D     X         3 85 6 Binarity among Cepheids in the Magellanic Clouds. SZABADOS L. and NEHEZ D.
2013A&A...550A..70G viz 16       D               2 201 45 Baade-Wesselink distances to Galactic and Magellanic Cloud Cepheids and the effect of metallicity. GROENEWEGEN M.A.T.
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 96       D     X         3 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.
2016ApJ...832..176I viz 16       D               1 3931 41 The panchromatic view of the Magellanic Clouds from classical Cepheids. I. Distance, reddening, and geometry of the Large Magellanic Cloud disk. INNO L., BONO G., MATSUNAGA N., et al.
2016A&A...595A...1G viz 17       D               1 3213 4492 The Gaia mission. GAIA COLLABORATION, PRUSTI T., DE BRUIJNE J.H.J., et al.
2017A&A...608A..85L 341       D     X C       8 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.
2016AcA....66..433U viz 16       D               1 2746 3 Gaia and Variable Stars. UDALSKI A., SOSZYNSKI I., SKOWRON D.M., et al.
2015AcA....65..297S viz 16       D               1 9695 105 The OGLE Collection of Variable Stars. Classical Cepheids in the Magellanic System. SOSZYNSKI I., UDALSKI A., SZYMANSKI M.K., et al.
2019A&A...622A..60C viz 17       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.
2021MNRAS.500..817C viz 17       D               1 5050 ~ The mid-infrared Leavitt law for classical Cepheids in the Magellanic Clouds. CHOWN A.H., SCOWCROFT V. and WUYTS S.

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