Cl* NGC 6362 SAW V41 , the SIMBAD biblio

Cl* NGC 6362 SAW V41 , the SIMBAD biblio (10 results) C.D.S. - SIMBAD4 rel 1.8 - 2024.04.25CEST07:22:48

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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
1999MNRAS.306..727M 39 19 Variable stars in the globular cluster NGC 6362. MAZUR B., KALUZNY J. and KRZEMINSKI W.
2014AcA....64..309K 212       D     X         6 42 10 The Clusters AgeS Experiment (CASE). Variable stars in the field of the globular cluster NGC 6362. KALUZNY J., THOMPSON I.B., ROZYCZKA M., et al.
2015AJ....150..155K 1709   K A D     X C       43 7 14 The Cluster AgeS Experiment (CASE). VII. Analysis of two eclipsing binaries in the globular cluster NGC 6362. KALUZNY J., THOMPSON I.B., DOTTER A., et al.
2017A&A...597A..87S 41           X         1 13 4 Evolutionary history of four binary blue stragglers from the globular clusters ω Cen, M 55, 47 Tuc, and NGC 6752. STEPIEN K., PAMYATNYKH A.A. and ROZYCZKA M.
2015ASPC..496..164S viz 16       D               1 196 98 DEBCat: A Catalog of Detached Eclipsing Binary Stars. SOUTHWORTH J.
2018ApJ...862...72V 576       S   X C       12 53 6 Constraints on the distance moduli, helium and metal abundances, and ages of globular clusters from their RR Lyrae and non-variable horizontal-branch stars. III. M55 and NGC 6362. VANDENBERG D.A. and DENISSENKOV P.A.
2018MNRAS.479.1953D 41           X         1 134 23 Testing models of stellar structure and evolution - I. Comparison with detached eclipsing binaries. DEL BURGO C. and ALLENDE PRIETO C.
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.
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.
2022MNRAS.509.4208V 493           X C F     9 16 4 Models for metal-poor stars with different initial abundances of C, N, O, Mg, and Si. II. Application to the colour-magnitude diagrams of the globular clusters 47 Tuc, NGC 6362, M 5, M 3, M 55, and M92. VANDENBERG D.A., CASAGRANDE L. and EDVARDSSON B.

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