| Literature DB >> 32455419 |
Robert D Stephens1, Brian D Warner2.
Abstract
CCD photometric observations of 10 main-belt asteroids were obtained from the Center for Solar System Studies from 2019 January to March. In light of recent period analysis, images of 2120 Tyumenia obtained in 2004 were re-examined. The resulting analysis found a period of 17.515 h, which is consistent with the recent results.Entities:
Year: 2019 PMID： 32455419 PMCID： PMC7243857
Source DB: PubMed Journal: Minor Planet Bull