Table 1
Various determinations of the parallax of ε Aur.
| Source | p (mas) | Notes | ||||
|
|
||||||
| Adams & Joy (1917) | 11–22 | 1 | ||||
| Adams & Joy (1917) | 60 | 2 | ||||
| Strand (1959) | 6 ± 4 | 3 | ||||
| Strand (1959) | 1 | 4 | ||||
| van de Kamp & Lippincott (1968) | 4 ± 2 | 5 | ||||
| van de Kamp (1978) | 1.72 ± 0.08 | 4 | ||||
| Heintz & Cantor (1994) | 3 ± 2 | 6 | ||||
| Heintz & Cantor (1994) | 1.65 ± 0.15 | 4 | ||||
| Perryman & ESA (1997) | 1.60 ± 1.16 | 7 | ||||
| van Leeuwen (2007a,b) | 1.53 ± 1.29 | 8 | ||||
Notes. Trigonometric parallaxes are quoted unless specified otherwise. 1... spectroscopic parallax; 2... by Jewdokimow at Yerkes; 3... 59 nights, Yerkes 1926−58; 4... comparing the semi-major axis from the astrometric and spectroscopic solutions; 5... 174 obs. at Sproul in 1938−56; 6... an extended series of the Sproul 363 night means over 44 years; 7... original Hipparcos parallax; 8... revised reduction of Hipparcos parallaxes.
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.