deletions | additions       diff --git a/sectionThe_Sample_la.tex b/sectionThe_Sample_la.tex  index d1eb2d9..be4a4c3 100644  --- a/sectionThe_Sample_la.tex  +++ b/sectionThe_Sample_la.tex 
...
do not confuse the picture because they are seen in spectral lines originating on the star's surface,  while the disk emits free-free emission from optically thin plasma.  The sample was constructed from the Be-star catalog of \cite{jaseck1982} \cite{Jaschek1998}  (in Vizier), by selecting northern (Dec$>$0) Be-stars with measured rotational velocities and no known (visual or spectroscopic) binary  companion. From this list the nearest exemplars. Our full target list (Table 1)  contains 52 Be-stars closer than 1 kpc, and includes all nearby "isolated'' Be-stars across the range of