|
other query modes : |
Identifier query |
Coordinate query |
Criteria query |
Reference query |
Basic query |
Script submission |
TAP |
Output options |
Object types |
Help |
| 2MASS J19544343+4039364 , the SIMBAD biblio (8 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.18CEST21:39:43 |
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 |
|---|---|---|---|---|---|---|---|---|---|
2013A&A...557L..10N 
|
15 | D | 1 | 12151 | 189 | Rotation periods of 12000 main-sequence Kepler stars: dependence on stellar spectral type and comparison with v sin i observations. | NIELSEN M.B., GIZON L., SCHUNKER H., et al. | ||
| 2017MNRAS.465.2294O | 170 | X C | 3 | 4 | 95 | A new asteroseismic diagnostic for internal rotation in γ Doradus stars. | OUAZZANI R.-M., SALMON S.J.A.J., ANTOCI V., et al. | ||
| 2017ApJ...851...39G | 40 | X | 1 | 17 | 19 | Gravity modes reveal the internal rotation of a post-mass-transfer Gamma Doradus/Delta Scuti hybrid pulsator in Kepler eclipsing binary KIC 9592855. | GUO Z., GIES D.R. and MATSON R.A. | ||
|
2018MNRAS.479..183B
|
16 | D | 1 | 2598 | 17 | Gaia luminosities of pulsating A-F stars in the Kepler field. | BALONA L.A. | ||
|
2019MNRAS.485.2380M
|
16 | D | 1 | 14330 | 108 | Gaia-derived luminosities of Kepler A/F stars and the pulsator fraction across the δ Scuti instability strip. | MURPHY S.J., HEY D., VAN REETH T., et al. | ||
|
2019A&A...626A.121O
|
17 | D | 1 | 40 | 62 | γ Doradus stars as a test of angular momentum transport models. | OUAZZANI R.-M., MARQUES J.P., GOUPIL M.-J., et al. | ||
|
2020MNRAS.491.3586L
|
16 | D | 2 | 609 | 75 | Gravity-mode period spacings and near-core rotation rates of 611 γ Doradus stars with Kepler. | LI G., VAN REETH T., BEDDING T.R., et al. | ||
|
2024A&A...684A.112F
|
18 | D | 1 | 491 | ~ | Age uncertainties of red giants due to cumulative rotational mixing of progenitors calibrated by asteroseismology. | FRITZEWSKI D.J., AERTS C., MOMBARG J.S.G., et al. |
