Reaching the boundary between stellar kinematic groups and very wide binaries - The Washington double stars with the widest angular separations

Free Access

Table 1:

Rejected wide binary candidates^a.
WDS	$\mu$	$d_{\rm phot}$	$d_{\rm spec}$	$d_\pi$	$V_{\rm r}$
identifier
00152+2454	No:	No	...	...	...
00400-1533	No:	No	...	...	...
00435+3351	No	No:	No	...	...
00520+2035	No	No	...	...	...
01163-3217	No:	No	...	...	...
03442-6448	No	No	No	No	No
07590-6338	No	No:	...	...	...
11125+3549	No	No	No	...	...
13410+6808	No:	No	No	...	...
13599+2520	No	No	No	...	...
20084+1503	No:	No	...	...	...
20302+2651	No	No	No	...	...

^a Coordinates are provided in Table A.1. The colon after ``No'' indicates that the corresponding parameters of stars in binary system candidates might be comparable if accounting for generous error bars.

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.