SV* HV 905 , the SIMBAD biblio

SV* HV 905 , the SIMBAD biblio (34 results) C.D.S. - SIMBAD4 rel 1.8 - 2024.04.25CEST14:27:57


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Title First 3 Authors
1972ATsir.671....1E 20 0 The composite period-age relation for Cepheids of the Magellanic Clouds, M 31 and Galaxy. EFREMOV Y.N.
1992PAZh...18..991K 41 ~ Studies of variable stars in the vicinity of the Large Magellanic Cloud star cluster NGC 1854. KUROCHKIN N.E.
1995ApJ...449..164S viz 37 26 Variable stars in Magellanic Cloud clusters. II. NGC 1850. SEBO K.M. and WOOD P.R.
1997ApJ...485L..25W 76 T                   3 38 Nonlinear models of the bump Cepheid HV 905 and the Large Magellanic Cloud distance modulus. WOOD P.R., ARNOLD A. and SEBO K.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.
1998MmSAI..69...99W 3 3 Deriving distances from nonlinear pulsation models of bump Cepheids. WOOD P.R.
1999ApJ...515....1S 153 47 The Hubble space telescope key project on the extragalactic distance scale. XIV. The cepheids in NGC 1365. SILBERMANN N.A., HARDING P., FERRARESE L., et al.
1999PASP..111.1539A 2 18 158 Calibration of the MACHO photometry database. ALCOCK C., ALLSMAN R.A., ALVES D.R., et al.
1999AcA....49..223U viz 1346 251 The Optical Lensing Experiment. Cepheids in the Magellanic Clouds. IV. Catalog of Cepheids from the Large Magellanic Cloud. UDALSKI A., SOSZYNSKI I., SZYMANSKI M., et al.
2000A&A...363..601A 4 8 Nonlinear model pulsations for long-period Cepheids. II. Magellanic Cloud Cepheids. AIKAWA T. and ANTONELLO E.
2002ApJ...565L..83B 4 5 67 Theoretical models for bump cepheids. BONO G., CASTELLANI V. and MARCONI M.
2002ApJ...578..144K 22 46 Large Magellanic Cloud bump cepheids: probing the stellar mass-luminosity relation. KELLER S.C. and WOOD P.R.
2002ApJS..142...71S viz 15       D               616 36 The cepheid period-luminosity relation in the Large Magellanic Cloud. SEBO K.M., RAWSON D., MOULD J., et al.
2005AJ....129.2257M 1 8 34 A "pulsational" distance determination for the Large Magellanic Cloud. MARCONI M. and CLEMENTINI G.
2006ApJ...642..834K 3 34 223 Bump Cepheids in the Magellanic clouds: metallicities, the distances to the LMC and SMC, and the pulsation-evolution mass discrepancy. KELLER S.C. and WOOD P.R.
2006MNRAS.369..723N viz 1172 22 Period-colour and amplitude-colour relations in classical Cepheid variables - IV. The multiphase relations. NGEOW C.-C. and KANBUR S.M.
2007A&A...474..557M 75           X         2 14 17 Modeling of RR Lyrae light curves: the case of M3. MARCONI M. and DEGL'INNOCENTI S.
2008AcA....58..163S viz 15       D               1 3398 282 The Optical Gravitational Lensing Experiment. The OGLE-III catalog of variable stars. I. Classical Cepheids in the Large Magellanic Cloud. SOSZYNSKI I., POLESKI R., UDALSKI A., et al.
2008AcA....58..313P viz 15       D               1 2950 15 Period changes of LMC Cepheids in the OGLE and MACHO Data. POLESKI R.
2012ApJ...748..107P viz 15       D               1 291 30 A global physical model for cepheids. PEJCHA O. and KOCHANEK C.S.
2014A&A...566A..37G viz 16       D               4 601 158 On the fine structure of the Cepheid metallicity gradient in the Galactic thin disk. GENOVALI K., LEMASLE B., BONO G., et al.
2015MNRAS.447.3342B viz 16       D               3 2329 21 On the variation of Fourier parameters for Galactic and LMC Cepheids at optical, near-infrared and mid-infrared wavelengths. BHARDWAJ A., KANBUR S.M., SINGH H.P., et al.
2015AJ....149..117M viz 16       D               1 1486 89 Large Magellanic Cloud near-infrared synoptic survey. I. Cepheid variables and the calibration of the Leavitt Law. MACRI L.M., NGEOW C.-C., KANBUR S.M., et al.
2016AJ....151...88B viz 16       D               1 1353 18 Large Magellanic Cloud near-infrared Synoptic Survey. II. The Wesenheit relations and their application to the distance scale. BHARDWAJ A., KANBUR S.M., MACRI L.M., et al.
2016ApJ...824...74G viz 16       D               1 1987 3 The influential effect of blending, bump, changing period, and eclipsing Cepheids on the Leavitt law. GARCIA-VARELA A., MUNOZ J.R., SABOGAL B.E., 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.
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.
2019ApJ...876...85R viz 37       D               1 75 1556 Large Magellanic Cloud Cepheid standards provide a 1% foundation for the determination of the Hubble constant and stronger evidence for physics beyond ΛCDM. RIESS A.G., CASERTANO S., YUAN W., et al.
2020MNRAS.491.4752B viz 17       D               1 13884 ~ When a period is not a full stop: Light-curve structure reveals fundamental parameters of Cepheid and RR Lyrae stars. BELLINGER E.P., KANBUR S.M., BHARDWAJ A., et al.
2020AJ....160..120J viz 17       D               1 365761 238 APOGEE data and spectral analysis from SDSS Data Release 16: seven years of observations including first results from APOGEE-South. JONSSON H., HOLTZMAN J.A., ALLENDE PRIETO C., 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.
2021ApJ...913...38B viz 17       D               1 2043 32 The influence of metallicity on the Leavitt law from geometrical distances of Milky Way and Magellanic Cloud Cepheids. BREUVAL L., KERVELLA P., WIELGORSKI P., et al.
2022A&A...658A..29R viz 18       D               1 72 23 The iron and oxygen content of LMC Classical Cepheids and its implications for the extragalactic distance scale and Hubble constant. Equivalent width analysis with Kurucz stellar atmosphere models. ROMANIELLO M., RIESS A., MANCINO S., et al.

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