An X-ray Jet in CH Cygni
Analysis of archival Chandra data
of the symbiotic system CH Cygni reveals faint extended
emission to the south, aligned with the optical and radio jets seen in
earlier HST and VLA observations.
CH Cygni is only the
second known white dwarf with an X-ray jet, after
R Aquarii.
Read the paper (ApJL 613, L61)