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| [BE74] 586 , the SIMBAD biblio (10 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.17CEST10:03:17 |
Sort references on where and how often the object is cited
trying to find the most relevant references on this object.
More on score
| 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 |
|---|---|---|---|---|---|---|---|---|---|
| 1963IrAJ....6..127L | 363 | 22 | Second list of emission-line objects in the Large Magellanic Cloud. | LINDSAY E.M. | |||||
| 1974A&AS...18...47B | 627 | 74 | H alpha emission-line stars in the Large Magellanic Cloud. I. A new deep survey. | BOHANNAN B. and EPPS H.W. | |||||
2002AJ....124.2039K 
|
1271 | 32 | Blue variable stars from the MACHO database. I. Photometry and spectroscopy of the Large Magellanic Cloud sample. | KELLER S.C., BESSELL M.S., COOK K.H., et al. | |||||
|
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. | ||
|
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. | ||
|
2012A&A...548A..16H
|
15 | D | 1 | 627 | 3 | Improved astrometry for the Bohannan & Epps catalogue. | HOWARTH I.D. | ||
|
2013A&A...555A.141H
|
15 | D | 3 | 1714 | 3 | Emission-line stars in the LMC: the Armagh survey and a metacatalogue. | HOWARTH I.D. | ||
|
2015MNRAS.454.1468K
|
16 | D | 2 | 2116 | 79 | Optically visible post-AGB stars, post-RGB stars and young stellar objects in the Large Magellanic Cloud. | KAMATH D., WOOD P.R. and VAN WINCKEL H. | ||
| 2022A&A...668A..22T | 102 | D | F | 3 | 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...671A..86D | 17 | D | 1 | 21 | 1 | Study of oxygen-rich post-AGB stars in the Milky Way as a means to explain the production of silicates among evolved stars. | DELL'AGLI F., TOSI S., KAMATH D., et al. |
