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IRAS F00471-7352 , the SIMBAD biblio (15 results) | C.D.S. - SIMBAD4 rel 1.8 - 2024.04.24CEST09:28:15 |
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. | |||||
2005A&A...438..521R | 1077 | 15 | Pulsation properties of C stars in the Small Magellanic Cloud. | RAIMONDO G., CIONI M.-R.L., REJKUBA M., et al. | |||||
2011AcA....61..217S | 15 | D | 1 | 2578 | 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 | 143671 | 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. | ||
2012ApJ...748...40B | 15 | D | 1 | 85 | 123 | The dust budget of the Small Magellanic Cloud: are asymptotic giant branch stars the primary dust source at low metallicity? | BOYER M.L., SRINIVASAN S., RIEBEL D., et al. | ||
2014MNRAS.439.2211K | 16 | 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. | ||
2015MNRAS.451.3504R | 16 | D | 1 | 212 | 33 | Spitzer infrared spectrograph point source classification in the Small Magellanic Cloud. | RUFFLE P.M.E., KEMPER F., JONES O.C., et al. | ||
2016MNRAS.457.2814S | 16 | D | 1 | 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. | ||
2016ApJ...826...44S | 16 | D | 1 | 237 | 24 | The infrared spectral properties of Magellanic carbon stars. | SLOAN G.C., KRAEMER K.E., McDONALD I., 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. | ||
2018A&A...609A.114G | 16 | D | 2 | 408 | 55 | Luminosities and mass-loss rates of Local Group AGB stars and red supergiants. | GROENEWEGEN M.A.T. and SLOAN G.C. | ||
2019A&A...626A..92G | 100 | D | C | 2 | 225 | ~ | 30-micron sources in galaxies with different metallicities. | GLADKOWSKI M., SZCZERBA R., SLOAN G.C., et al. | |
2019ApJ...887...82K | 17 | D | 1 | 263 | ~ | Stellar pulsation and the production of dust and molecules in galactic carbon stars. | KRAEMER K.E., SLOAN G.C., KELLER L.D., et al. | ||
2020A&A...636A..48G | 17 | 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. | ||
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. |