aud -s type
uses directly the output of the previous
command aud
as input to
prepare the new list of star number, instead of the original sample.
This possibility is useful when the number of stars of the new sample becomes smaller than that of the initial sample.
ubv ref -eq 1341
aud vsn
aud -s mk
ubv
selects the data from
reference 1341, then aud vsn
gets the Vsini data, which are less
numerous, and aud -s mk
looks for the spectral types of the stars
in the new sample.