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Tue Aug 10, 2004

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)

Labels: 2004, /jets