UCAC3 127-192903 , the SIMBAD biblio

UCAC3 127-192903 , the SIMBAD biblio (11 results) C.D.S. - SIMBAD4 rel 1.8 - 2024.04.17CEST00:33:37


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Title First 3 Authors
2004ApJ...609..755B 45 54 X-ray sources and their optical counterparts in the globular cluster M4. BASSA C., POOLEY D., HOMER L., et al.
2013AJ....145...43K viz 2341   K A D     X   F     60 13 28 The Cluster AgeS Experiment (CASE). V. Analysis of three eclipsing binaries in the globular cluster M4. KALUZNY J., THOMPSON I.B., ROZYCZKA M., et al.
2013AcA....63..181K 250       D     X         7 36 17 The Clusters AgeS Experiment (CASE) variable stars in the globular cluster M4. KALUZNY J., THOMPSON I.B., ROZYCZKA M., et al.
2014PASP..126..521S viz 16       D               1 96 31 Optical and near-infrared UBVRIJHK photometry for the RR Lyrae stars in the nearby globular cluster M 4 (NGC 6121). STETSON P.B., BRAGA V.F., DALL'ORA M., et al.
2014MNRAS.444.2525C 18       D               2 96 425 Improving PARSEC models for very low mass stars. CHEN Y., GIRARDI L., BRESSAN A., et al.
2015AJ....149..131E viz 16       D               3 213 106 Main-sequence effective temperatures from a revised mass-luminosity relation based on accurate properties. EKER Z., SOYDUGAN F., SOYDUGAN E., et al.
2014PASA...31...24E viz 16       D               1 258 57 The catalogue of stellar parameters from the detached double-lined eclipsing binaries in the Milky Way. EKER Z., BILIR S., SOYDUGAN F., et al.
2015ASPC..496..164S viz 16       D               1 196 98 DEBCat: A Catalog of Detached Eclipsing Binary Stars. SOUTHWORTH J.
2018MNRAS.479.5491E viz 16       D               2 301 126 Interrelated main-sequence mass-luminosity, mass-radius, and mass-effective temperature relations. EKER Z., BAKIS V., BILIR S., et al.
2017PASJ...69...79L 41           X         1 29 17 Comprehensive photometric study of an extremely low mass ratio deep contact binary in the globular cluster M 4 . LI K., HU S., CHEN X., et al.
2019A&A...625A..68S viz 84             C       1 342 126 The CARMENES search for exoplanets around M dwarfs. Different roads to radii and masses of the target stars. SCHWEITZER A., PASSEGGER V.M., CIFUENTES C., et al.

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