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| OGLE SMC-LPV-13055 , the SIMBAD biblio (8 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.16CEST10:55:32 |
| 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 |
|---|---|---|---|---|---|---|---|---|---|
|
2011AcA....61..217S |
15 | D | 1 | 19389 | 94 | The Optical Gravitational Lensing Experiment. The OGLE-III catalog of variable stars. XIII. Long-period variables in the Small Magellanic Cloud. | SOSZYNSKI I., UDALSKI A., SZYMANSKI M.K., et al. | ||
|
2011AJ....142..103B |
15 | D | 1 | 143670 | 153 | Surveying the agents of galaxy evolution in the tidally stripped, low metallicity Small Magellanic Cloud (SAGE-SMC). II. Cool evolved stars. | BOYER M.L., SRINIVASAN S., VAN LOON J.Th., et al. | ||
|
2014MNRAS.439.2211K |
15 | D | 1 | 380 | 94 | Optically visible post-AGB/RGB stars and young stellar objects in the Small Magellanic Cloud: candidate selection, spectral energy distributions and spectroscopic examination. | KAMATH D., WOOD P.R. and VAN WINCKEL H. | ||
|
2016MNRAS.457.2814S |
252 | D | X F | 6 | 8923 | 34 | The evolved-star dust budget of the Small Magellanic Cloud: the critical role of a few key players. | SRINIVASAN S., BOYER M.L., KEMPER F., et al. | |
|
2017ApJ...834..185K |
16 | D | 1 | 265 | 14 | Characterizing the population of bright infrared sources in the Small Magellanic Cloud. | KRAEMER K.E., SLOAN G.C., WOOD P.R., et al. | ||
|
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. | ||
| 2022A&A...668A..22T | 911 | D | S X C F | 19 | 19 | 2 | Understanding dust production and mass loss in the AGB phase using post-AGB stars in the Magellanic Clouds. | TOSI S., DELL'AGLI F., KAMATH D., et al. | |
| 2023A&A...673A..41T | 17 | D | 1 | 29 | ~ | A study of carbon-rich post-AGB stars in the Milky Way to understand the production of carbonaceous dust from evolved stars. | TOSI S., KAMATH D., DELL'AGLI F., et al. |