Table A.1.
Average pV-values of potential X-complex families.
Asteroid Family | Location | pV |
---|---|---|
87 Sylvia | OMB | 0.078 |
161 Athor | IMB | 0.184 |
293 Brasilia | OMB | 0.081 |
322 Phaeo | CMB | 0.077 |
363 Padua | CMB | 0.076 |
396 Aeolia | CMB | 0.083 |
369 Aeria | CMB | 0.081 |
589 Croatia | OMB | 0.073 |
689 Zita | IMB | 0.177 |
709 Fringilla | OMB | 0.075 |
909 Ulla | OMB | 0.057 |
1222 Tina | CMB | 0.076 |
1303 Luthera | OMB | 0.072 |
5567 Durisen | OMB | 0.076 |
7481 San Marcello | OMB | 0.177 |
Notes. Reported average pV-values for the Athor and Zita families are the ones that were retrieved using the original family membership by Delbo et al. (2019) and before a re-assessment of the family membership, which was performed after our observations. Column location refers to the region of the main belt where the family is located following Nesvorny et al. (2015), namely IMB = Inner Main Belt, 2.0 < a< 2.5 au, i< 17.5°; CMB = Central Main Belt, 2.5 < a< 2.82 au, i< 17.5°; OMB = Outer Main Belt, 2.82 < a< 3.7 au, i< 17°, where a and i are the orbital semi-major axis and inclination.
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.