  We explore the similarities between accreting white dwarfs (CH Cyg and MWC
560) and the much more energetic jet sources - quasars and microquasars.
To-date we have identified several common attributes: (1) they exhibit
collimated outflows (jets); (2) the jets are precessing; (3) these two
symbiotic stars exhibit quasar-like emission line spectra; (4) there is a
disk-jet connection like that observed in microquasars. Additionally they may
have a similar energy source (extraction of rotational energy from the
accreting object). Study of the low energy analogues could have important
implications for our understanding of their higher energy cousins.
