2MASS J05140595-6915568 , the SIMBAD biblio

2MASS J05140595-6915568 , the SIMBAD biblio (21 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.18CEST21:41:30

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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
2008AJ....136.1242F viz 15       D               1 47759 44 The properties of long-period variables in the Large Magellanic Cloud from MACHO. FRASER O.J., HAWLEY S.L. and COOK K.H.
2011A&A...536A..60S viz 15       D               1 43415 15 Long period variables in the Large Magellanic Cloud from the EROS-2 survey. SPANO M., MOWLAVI N., EYER L., et al.
2013Natur.495...76P 31 9 569 An eclipsing-binary distance to the Large Magellanic Cloud accurate to two per cent. PIETRZYNSKI G., GRACZYK D., GIEREN W., et al.
2013A&A...558A..51Z 15       D   O           1 42 8 Apsidal motion and absolute parameters for five LMC eccentric eclipsing binaries. ZASCHE P. and WOLF M.
2015ApJ...812...96G 211       D     X         6 77 20 Beyond the main sequence: testing the accuracy of stellar masses predicted by the PARSEC evolutionary tracks. GHEZZI L. and JOHNSON J.A.
2016AJ....152...29E 79               F     1 11 7 The orbital and physical parameters, and the distance of the eclipsing binary system OGLE-LMC-ECL-25658 in the Large Magellanic Cloud. ELGUETA S.S., GRACZYK D., GIEREN W., et al.
2016A&A...592A..15C 17       D     X         1 36 78 The dependence of convective core overshooting on stellar mass. CLARET A. and TORRES G.
2016ApJ...832..176I viz 55       D     X         2 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.
2017MNRAS.468.3533E 214       D     X         6 73 9 Models for 60 double-lined binaries containing giants. EGGLETON P.P. and YAKUT K.
2017ApJ...849...18C 135       D     X         4 38 31 The dependence of convective core overshooting on stellar mass: a semi-empirical determination using the diffusive approach with two different element mixtures. CLARET A. and TORRES G.
2015ASPC..496..164S viz 16       D               1 197 98 DEBCat: A Catalog of Detached Eclipsing Binary Stars. SOUTHWORTH J.
2018ApJ...860....1G viz 522     A D S   X C       12 26 13 The late-type eclipsing binaries in the Large Magellanic Cloud: catalog of fundamental physical parameters. GRACZYK D., PIETRZYNSKI G., THOMPSON I.B., et al.
2018MNRAS.479.1953D 40           X         1 134 23 Testing models of stellar structure and evolution - I. Comparison with detached eclipsing binaries. DEL BURGO C. and ALLENDE PRIETO C.
2018A&A...618A.177C 217       D     X C       5 12 11 Significant uncertainties from calibrating overshooting with eclipsing binary systems. CONSTANTINO T. and BARAFFE I.
2019A&A...622A..63G 99 ~ The VMC Survey. XXXIII. The tip of the red giant branch in the Magellanic Clouds. GROENEWEGEN M.A.T., CIONI M.-R.L., GIRARDI L., et al.
2019Natur.567..200P 21       D               1 62 351 A distance to the Large Magellanic Cloud that is precise to one per cent. PIETRZYNSKI G., GRACZYK D., GALLENNE A., et al.
2019MNRAS.485.4641C 16       D               1 40 37 Mixing by overshooting and rotation in intermediate-mass stars. COSTA G., GIRARDI L., BRESSAN A., et al.
2019ApJ...876..134C 545       D S   X C       12 31 55 The dependence of convective core overshooting on stellar mass: reality check and additional evidence. CLARET A. and TORRES G.
2020ApJ...889..179G 16       D               1 98 38 Empirical calibration of the reddening maps in the Magellanic Clouds. GORSKI M., ZGIRSKI B., PIETRZYNSKI G., et al.
2021ApJS..255....1B viz 17       D               1 498270 9 Classification of OGLE eclipsing binary stars based on their morphology type with locally linear embedding. BODI A. and HAJDU T.
2021MNRAS.507.1795R 142       D     X   F     3 28 ~ Determining fundamental parameters of detached double-lined eclipsing binary systems via a statistically robust machine learning method. REMPLE B.A., ANGELOU G.C. and WEISS A.

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