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| V* V653 Sco , the SIMBAD biblio (9 results) | C.D.S. - SIMBAD4 rel 1.8 - 2024.04.18CEST12:48:15 |
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 |
|---|---|---|---|---|---|---|---|---|---|
2012A&A...539A..51T 
|
93 | D | O X | 3 | 1670 | 28 | Tracking down R coronae Borealis stars from their mid-infrared WISE colours. | TISSERAND P. | |
| 2012ApJ...755...98M | 77 | C | 3 | 54 | 13 | Discovery of bright galactic R Coronae Borealis and DY Persei variables: rare GEMS mined from ACVS. | MILLER A.A., RICHARDS J.W., BLOOM J.S., et al. | ||
| 2013A&A...551A..77T | 172 | D | O X C | 4 | 173 | 27 | The ongoing pursuit of R Coronae Borealis stars: the ASAS-3 survey strikes again. | TISSERAND P., CLAYTON G.C., WELCH D.L., et al. | |
|
2020A&A...635A..14T
|
17 | D | O | 1 | 206 | 21 | A plethora of new R Coronae Borealis stars discovered from a dedicated spectroscopic follow-up survey. | TISSERAND P., CLAYTON G.C., BESSELL M.S., et al. | |
|
2022ApJS..260...46I
|
18 | D | 1 | 65989 | 11 | The OGLE Collection of Variable Stars: Nearly 66,000 Mira Stars in the Milky Way. | IWANEK P., SOSZYNSKI I., KOZLOWSKI S., et al. | ||
|
2022A&A...667A..84K
|
18 | D | 2 | 79 | 3 | R Coronae Borealis and dustless hydrogen-deficient carbon stars likely have different oxygen isotope ratios. | KARAMBELKAR V., KASLIWAL M.M., TISSERAND P., et al. | ||
|
2022A&A...667A..85C
|
18 | D | 1 | 156 | ~ | Peculiar hydrogen-deficient carbon stars: strontium-rich stars and the s-process. | CRAWFORD C.L., TISSERAND P., CLAYTON G.C., et al. | ||
| 2023RNAAS...7..147P | 261 | A | X C | 5 | 3 | ~ | New Dimming Events in Southern R Coronae Borealis Stars. | PEARCE A., LOVE T., VELEZ P., et al. | |
|
2023A&A...677A.137M
|
19 | D | 1 | 94 | ~ | Stellar variability in Gaia DR3 I. Three-band photometric dispersions for 145 million sources. | MAIZ APELLANIZ J., HOLGADO G., PANTALEONI GONZALEZ M., et al. |
