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| OGLE LMC-LPV-15419 , the SIMBAD biblio (19 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.15CEST12:37:04 |
| 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 |
|---|---|---|---|---|---|---|---|---|---|
|
2001AJ....122.1844E |
1825 | 79 | MSX, 2MASS, and the Large Magellanic Cloud: a combined near- and mid-infrared view. | EGAN M.P., VAN DYK S.D. and PRICE S.D. | |||||
|
2008AJ....136...18W |
15 | D | 1 | 1226 | 186 | Spitzer SAGE survey of the Large Magellanic Cloud. III. Star formation and ∼1000 new candidate young stellar objects. | WHITNEY B.A., SEWILO M., INDEBETOUW R., et al. | ||
|
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. | ||
|
2009AcA....59..239S |
15 | D | 1 | 92001 | 185 | The Optical Gravitational Lensing Experiment. The OGLE-III catalog of variable stars. IV. Long-period variables in the Large Magellanic Cloud. | SOSZYNSKI I., UDALSKI A., SZYMANSKI M.K., et al. | ||
|
2010PASP..122..683K |
15 | D | 1 | 238 | 89 | The SAGE-Spec Spitzer Legacy program: the life cycle of dust and gas in the Large Magellanic Cloud. | KEMPER F., WOODS P.M., ANTONIOU V., et al. | ||
| 2011ApJ...728...93S | 39 | X | 1 | 25 | 70 | The mass-loss return from evolved stars to the Large Magellanic Cloud. IV. Construction and validation of a grid of models for oxygen-rich AGB stars, red supergiants, and extreme AGB stars. | SARGENT B.A., SRINIVASAN S. and MEIXNER M. | ||
|
2011MNRAS.411.1597W |
53 | D | X | 2 | 230 | 107 | The SAGE-Spec Spitzer Legacy programme: the life-cycle of dust and gas in the Large Magellanic Cloud – point source classification I. | WOODS P.M., OLIVEIRA J.M., KEMPER F., et al. | |
|
2011A&A...530A..90V |
15 | D | 1 | 1414 | 46 | The optically bright post-AGB population of the LMC. | VAN AARLE E., VAN WINCKEL H., LLOYD EVANS T., et al. | ||
|
2011A&A...536A..60S |
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. | ||
|
2012MNRAS.427.3209J |
15 | D | 1 | 293 | 40 | On the metallicity dependence of crystalline silicates in oxygen-rich asymptotic giant branch stars and red supergiants. | JONES O.C., KEMPER F., SARGENT B.A., et al. | ||
|
2014MNRAS.440..631J |
15 | D | 1 | 151 | 22 | Modelling the alumina abundance of oxygen-rich evolved stars in the Large Magellanic Cloud. | JONES O.C., KEMPER F., SRINIVASAN S., et al. | ||
|
2016AJ....151..146C |
16 | D | 1 | 787 | 1 | A systematic search for the spectra with features of crystalline silicates in the Spitzer IRS enhanced products. | CHEN R., LUO A., LIU J., et al. | ||
|
2016AJ....152..164H |
16 | D | 1 | 887 | 7 | Period estimation for sparsely-sampled quasi-periodic light curves applied to Miras. | HE S., YUAN W., HUANG J.Z., et al. | ||
|
2018A&A...609A.114G |
16 | D | 408 | 55 | Luminosities and mass-loss rates of Local Group AGB stars and red supergiants. | GROENEWEGEN M.A.T. and SLOAN G.C. | |||
|
2019ApJ...884...20B |
16 | D | 1 | 1729 | ~ | Multiwavelength period-luminosity and period-luminosity-color relations at maximum light for Mira variables in the Magellanic Clouds. | BHARDWAJ A., KANBUR S., HE S., et al. | ||
|
2021ApJ...919...99I |
17 | D | 2 | 1667 | 10 | Mid-infrared period-luminosity relations for Miras in the Large Magellanic Cloud. | IWANEK P., SOSZYNSKI I. and KOZLOWSKI S. | ||
|
2021A&A...656A..66T |
17 | D | 1 | 14341 | 8 | Semi-regular red giants as distance indicators. I. The period-luminosity relations of semi-regular variables revisited. | TRABUCCHI M., MOWLAVI N. and LEBZELTER T. | ||
|
2022AJ....163..192O |
17 | D | 1 | 1483 | 5 | Difference of Photometric Properties between Regular and Nonregular Miras in the Magellanic Clouds. | OU J.-Y. and NGEOW C.-C. | ||
|
2023A&A...674A..15L |
17 | D | 1 | 1720610 | 15 | Gaia Data Release 3 The second Gaia catalogue of long-period variable candidates. | LEBZELTER T., MOWLAVI N., LECOEUR-TAIBI I., et al. |