Table 1
Stellar parameters used for HD 139614.
d(1,2) [pc] | ![]() |
SpTyp(4) | ![]() |
![]() |
![]() |
log g(5) | Age(6) [Myr] |
|
|||||||
140 ± 27 | 0.09 | A7V | 1.7 ± 0.3 | 1.6 | 3.895 | 4.0 |
![]() |
Notes. The uncertainties are taken from the references given below. The stellar radius R∗ was derived from the stellar luminosity and T∗ taken from van Boekel et al. (2005); no uncertainty is available, but it is consistent with other radius estimates (e.g., Alecian et al. 2013). The log g and M∗ values are consistent with our derived R∗ value (see, e.g., Alecian et al. 2013).
Reference. (1) de Zeeuw et al. (1999); (2) Preibisch & Mamajek (2008); (3) Yudin et al. (1999); (4) van Boekel et al. (2005); (5) Sylvester et al. (1997); (6) Alecian et al. (2013).
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.