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2MASS J05140595-6915568 , the SIMBAD biblio (21 results) | C.D.S. - SIMBAD4 rel 1.8 - 2024.03.28CET09:42:58 |
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 | 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 | 15 | D | 1 | 43434 | 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 | 16 | D | O | 1 | 42 | 8 | Apsidal motion and absolute parameters for five LMC eccentric eclipsing binaries. | ZASCHE P. and WOLF M. | |
2015ApJ...812...96G | 214 | 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 | 80 | 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 | 18 | D | X | 1 | 36 | 78 | The dependence of convective core overshooting on stellar mass. | CLARET A. and TORRES G. | |
2016ApJ...832..176I | 56 | 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 | 219 | D | X | 6 | 73 | 9 | Models for 60 double-lined binaries containing giants. | EGGLETON P.P. and YAKUT K. | |
2017ApJ...849...18C | 138 | 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 | 16 | D | 1 | 196 | 98 | DEBCat: A Catalog of Detached Eclipsing Binary Stars. | SOUTHWORTH J. | ||
2018ApJ...860....1G | 535 | 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 | 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. | ||
2018A&A...618A.177C | 222 | 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 | 22 | 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 | 17 | D | 1 | 40 | 37 | Mixing by overshooting and rotation in intermediate-mass stars. | COSTA G., GIRARDI L., BRESSAN A., et al. | ||
2019ApJ...876..134C | 561 | 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 | 17 | 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 | 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 | 148 | 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. |