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| OGLE LMC-LPV-81113 , the SIMBAD biblio (10 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.15CEST22:04:06 |
| 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 |
|---|---|---|---|---|---|---|---|---|---|
|
2004A&A...425..595G |
2919 | 66 | Long Period Variables in the Magellanic Clouds: OGLE + 2MASS + DENIS. | GROENEWEGEN M.A.T. | |||||
|
2009AJ....137.3139V |
15 | D | 1 | 1973 | 42 | Variable evolved stars and young stellar objects discovered in the large Magellanic cloud using the SAGE survey. | VIJH U.P., MEIXNER M., BABLER B., et al. | ||
|
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. | ||
|
2012A&A...539A..51T |
15 | D | 1 | 1670 | 28 | Tracking down R coronae Borealis stars from their mid-infrared WISE colours. | TISSERAND P. | ||
|
2017AJ....154..149Y |
16 | D | 1 | 692 | 33 | Large Magellanic Cloud near-infrared synoptic survey. V. Period-Luminosity relations of Miras. | YUAN W., MACRI L.M., HE S., et al. | ||
|
2020A&A...636A..48G |
16 | D | 1 | 970 | ~ | The VMC Survey. XXXVII. Pulsation periods of dust-enshrouded AGB stars in the Magellanic Clouds. | GROENEWEGEN M.A.T., NANNI A., CIONI M.-R.L., 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...669A..60P |
17 | D | 1 | 110 | 1 | Do Miras show long secondary periods? | PAWLAK M. |