X-Ray Observation of a Transient Symbiotic-Star Jet

Details X-Ray Observation of a Transient Symbiotic-Star Jet X-Ray Observation of a Transient Symbiotic-Star Jet

Sep 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005cxo..prop.1915s&link_type=abstract

Chandra Proposal ID #07300767

Astronomy and Astrophysics

Astrophysics

Chandra Proposal Id #07300767

Scientific paper

Astrophysical jets are ubiquitous in the universe, yet the collimation and acceleration mechanisms for these outflows are unclear. Accretion disks, however, are likely to play a key role. White dwarfs have possibly the best-understood disks, so symbiotic stars (SS), which are a recently identified class of jet-producing objects, are promising targets. The two SS X-ray jets that have been discovered to date (R Aqr and CH Cyg) both show X-ray structure more extended than their radio jets. To further study the X-ray properties of SS jets, most of which are transient, plus investigate changes in the central object when a jet in ejected, we propose a Chandra TOO observation (slow turn-around) of the next SS jet that is discovered. This proposal was accepted in AO5 and AO6, but not triggered.

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