- ...1,
- Present address: Ohio State University, Columbus, Ohio.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
- ...1,
- Present address: Joint Astronomy Centre, Hilo, Hawaii.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
- ... radiation
- For low-excitation lines this may not be entirely correct, but we estimate that the additional error introduced will be no more than 20% for
K.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
- ... meanings
- As
has been approximated by 
in this formula, a factor of
1.06, which relates the integrated intensity of a Gaussian profile to the FWHM, has been neglected.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.