A spectroscopic survey of the youngest field stars in the solar neighbourhood - I. The optically bright sample

Free Access

Table 4:

Consistency of the stellar parameters derived from the *Aurelie* (left) and *Elodie* (right) spectrographs.
RasTyc Name	RV (km s^-1)		$v\sin i$ (km s^-1)		$T_{\rm eff}$ (K)		$\log g$		[Fe/H]
RasTyc 2100+4530	-23.3	-23.1	6	6	5720	5730	4.23	4.42	-0.01	0.01
RasTyc 2114+3941	-10.8	-11.2	24	27	5730	5730	4.14	4.28	-0.23	-0.53
RasTyc 2118+2613	-16.3	-16.8	7	6	5230	5330	4.31	4.52	-0.09	-0.10
RasTyc 2132+3605	-6.2	-6.8	5	4	5140	5000	3.20	2.84	-0.03	-0.05
RasTyc 2137+1946	-5.2	-6.0	4	3	4900	4870	3.03	2.85	0.04	-0.01

Source LaTeX | All tables | In the text

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.