Motion in the R-Aquarii Jet 1991, 1992, 1993: Image Deconvolution of 1992 Data
Images from the Hubble Space Telescope's Faint Object Camera from 1991, 1992, and 1993 demonstrate motion in the R Aquarii emission jet. Since images from this period were still affected by the primary mirror flaw, the images were restored to the original design resolution using the maximum entropy method.
An animation of the deconvolution of a 1992 image of R-Aquarii jet from the Hubble Space Telescopes Faint Object Camera.
Video slate image reads "Image Deconvolution 1992 data only".
Credits
Please give credit for this item to:
NASA/Goddard Space Flight Center
Scientific Visualization Studio
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Animators
- Shahram Shiri (NASA)
- Pamela ONeil (NASA)
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Scientists
- J. Michael Hollis (NASA/GSFC)
- Richard Lyon (NASA/GSFC)
- John E. Dorband (NASA/GSFC)
- W. A. Feibelman (NASA/GSFC)
Release date
This page was originally published on Sunday, June 4, 1995.
This page was last updated on Wednesday, May 3, 2023 at 2:00 PM EDT.
Series
This page can be found in the following series:Related papers
J. M. Hollis, R. G. Lyon, J. E. Dorband, W. A. Feibelman, Motion of the Ultraviolet R Aquarii Jet, ApJ, 475, 231-236.
J. M. Hollis, R. G. Lyon, J. E. Dorband, W. A. Feibelman, Motion of the Ultraviolet R Aquarii Jet, ApJ, 475, 231-236.
Datasets used
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[HST: FOC]
ID: 37 -
[HST: WFPC2]
ID: 655Wide-Field Planetary Camera 2 (WFPC2) was installed in Dec 1993 and used to obtain high resolution images of astronomical objects. This camera was removed in the last servicing mission so it is no longer in service.
This dataset can be found at: http://www.stsci.edu/hst/wfpc2/wfpc2_diag.html
See all pages that use this dataset
Note: While we identify the data sets used on this page, we do not store any further details, nor the data sets themselves on our site.