- ... clumps
- Appendix A is only available in electronic form at http://www.aanda.org
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
- ...1,
- Present address: Harvard-Smithsonian Centre for Astrophysics.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
- ... telescope
- IRAM is an international institute for research in millimeter astronomy. IRAM is supported by INSU/CNRS
(France), MPG (Germany) and IGN (Spain).
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
- ... telescope
- Based on observations with the 100 m telescope of the
MPIfR(Max-Planck-Institut für Radioastronomie) at Effelsberg).
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
- ... given
- Table A.2, available in electronic form, contains the following information. Column 1 lists the name of the source, Cols. 2 and 5 gives the
(1, 1) and (2, 2) main beam brightness temperature respectively, Col. 3 gives the (1, 1) line width, and Col. 4 lists the (1, 1) main group optical depth. In Table A.3 we list the sources observed in
,
the integrated line intensity, FWHM of the line and the total optical depth from Cols. 1 to 4.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
- ...
- Table A.4, available in electronic form, contains the following information. Column 1 lists the name of the source, Cols. 2 and 3 gives the
(1-0) and (2-1) integrated intensity.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.