Astrometry of the optical jet of M 87

Details Astrometry of the optical jet of M 87 Astrometry of the optical jet of M 87

Jan 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990pazh...16...18m&link_type=abstract

Pis'ma v Astronomicheskii Zhurnal (ISSN 0320-0108), vol. 16, Jan. 1990, p. 18-23. In Russian. In Russian. In Russian.

Astronomy and Astrophysics

Astronomy

Astrometry, Astronomical Photography, Elliptical Galaxies, Image Processing, Light Emission, Angular Resolution, Linear Filters, Maximum Entropy Method, Photographic Plates, Photographic Processing

Scientific paper

Photographic plates of M 87 obtained with a 6-m telescope have been processed using the digital maximum entropy method and linear filtering. An optical image of the jet of M 87 with an angular resolution of 0.8 arcsec was obtained. It is found that the optical knots significantly deviate from the jet axis near the galaxy nucleus. The knots A and C were resolved into separate details across the axis. The positions of the optical knots are measured and compared with radio data.

Affiliated with

Also associated with

No associations

Rating

Astrometry of the optical jet of M 87 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 Astrometry of the optical jet of M 87, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Astrometry of the optical jet of M 87 will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1564244