Table 1
Stellar parameters for HD 175607.
| Parameter | Value | Note |
|
|
||
| RA [h m s] | 19 01 05.49 | (1) |
| Dec [d m s] | –66 11 33.65 | (1) |
| Spectral type | G6V | |
| mv | 8.61 | |
| B−V | 0.70 | |
| Parallax [mas] | 22.09±1.01 | (1) |
| Distance [pc] | 45.27±2.07 | |
| Teff [K] | 5392±17 | (2) |
| log g | 4.64±0.03 | (2) |
| [Fe/H] | −0.62±0.01 | (2) |
| [α/ Fe] | 0.26 | (3) |
| Mass [M⊙] | 0.74±0.05 | (4) |
| Radius [R⊙] | 0.71±0.03 | (4) |
| Mass [M⊙] | 0.71±0.01 | (5) |
| Radius [R⊙] | 0.70±0.01 | (5) |
| Age [Gyr] | 10.32±1.58 | (5) |
|
−4.92 | |
| PRot [days] | 28.95±0.33 | (6) |
| PRot [days] | 29.68±0.47 | (7) |
| v sini [km s-1] | 0.9 | (8) |
| v sini [km s-1] | 1.31 | (9) |
Reference. (1) van Leeuwen (2007); (2) Sousa et al. (2011a), with the surface gravity corrected following Mortier et al. (2014); (3) Adibekyan et al. (2012c); (4) using the Torres et al. (2010) calibration; (5) Bayesian estimation (da Silva et al. 2006) using the PARSEC isochrones (Bressan et al. 2012); (6) using the empirical relationships from Noyes et al. (1984, their Eqs. (3) and (4)); (7) using the empirical relationship from Mamajek & Hillenbrand (2008, their Eq. (5)); (8) Glebocki & Gnacinski (2005); (9) using the recipe of Santos et al. (2002), adapted to the HARPS CCF.
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