All Tables

Table 1: Spectra used for AG Peg.
Table 2: IUE spectra used for the selected symbiotic stars.
Table 3: The distribution of emission lines for AG Peg, according to population processes.
Table 4: The broad emission lines in AG Peg spectra.
Table 5: Pumped Fe II channels confirmed by 3 or more fluorescence lines.
Table 6: Pumped channels in ions other than Fe II.
Table 7: Parity forbidden lines observed in AG Peg.
Table 8: The relative line strengths of the Fe II multiplet a⁶D-z⁶D.
Table 9: The nature of lines having white dwarf wind profile in AG Peg in symbiotic stars.
Table 10: Fe II emission in symbiotic stars.
Table 11: Forbidden lines searched for in 20 symbiotic stars.
Table 12: Forbidden spectra in symbiotic stars.
Table 13: A sample of the AG Peg line list.
Full Version
Table 13: All emission lines observed in AG Peg.
Table 14: Intensities of emission lines not detectable with LWP25995 or SWP47715.
Table 15: Emission lines saturated in LWP25995 or SWP47715.
Table 16: Aborption lines in AG Peg.