Details on Acronym: [CTS2017] | |
| [CTS2017] | (Collins+Tollerud+Sand+, 2017) |
| Write: | <<[CTS2017] NN>> |
| N: | 28 |
| Object: | * (SIMBAD class: Star) |
| Note: | Keck II DEIMOS spectro-photometric observations of N=28 stars in the field of Leo V dwarf galaxy. See also [WBE2009]. |
| in source: | NAME Leo V |
| Ref: | =2017MNRAS.467..573C |
| by | COLLINS M.L.M. , TOLLERUD E.J., SAND D.J., BONACA A., WILLMAN B., STRADER J. |
| Mon. Not. R. Astron. Soc., 467, 573-585 (2017) | |
| Dynamical evidence for a strong tidal interaction between the Milky Way and its satellite, Leo V. | |
| o | Table 1: <[CTS2017] NN> N=28 among (Nos 10-62). |
| Origin | of the Acronym: S = Created by Simbad, the CDS Database |