Comparing restored HST and VLA imagery of R Aquarii

Details Comparing restored HST and VLA imagery of R Aquarii Comparing restored HST and VLA imagery of R Aquarii

Feb 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992apj...386..293h&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 386, Feb. 10, 1992, p. 293-298.

Astronomy and Astrophysics

Astronomy

22

Hubble Space Telescope, Symbiotic Stars, Very Large Array (Vla), Astronomical Observatories, Image Processing, Maximum Entropy Method, Radio Astronomy

Scientific paper

The maximum entropy method is applied to Hubble Space Telescope data taken of the R Aquarii binary system and its jet with the Faint Object Camera in order to restore an image in forbidden O III at 5007 A plagued by spherical aberration and detector saturation. These results are compared with 2-cm radio continuum imagery taken with the Very Large Array at the same limiting resolution of about 0.1 arcsec. The comparison suggests that shock excitation of the inner jet accounts for a spatial difference between the forbidden O III and radio continuum emission regions.

Affiliated with

Also associated with

No associations

Rating

Comparing restored HST and VLA imagery of R Aquarii does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Comparing restored HST and VLA imagery of R Aquarii, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Comparing restored HST and VLA imagery of R Aquarii will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1046476