VLBI detection of SS433

Details VLBI detection of SS433 VLBI detection of SS433

Nov 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979a%26a....79l..26s&link_type=abstract

Astronomy and Astrophysics, vol. 79, no. 3, Nov. 1979, p. L26, L27.

Astronomy and Astrophysics

Astronomy

9

Extragalactic Radio Sources, Radio Astronomy, Very Long Base Interferometry, Flux Density

Scientific paper

Observations at 6 cm of SS433 using a 3-station VLBI network which had linear resolutions of between 1 and 3 x 10 to the 15th cm at the estimated distance of the object indicate an angular structure of approximately 10 milli-arcseconds or 10 to the 15th cm at 3.5 kpc, and there is a weak indication that the structure is not circularly symmetric. It is suggested that SS433 could be a mini extended double radio source such as ScoX-1. The elements of the interferometer system were the 1.6 km Westerbork synthesis radio telescope used as an adding interferometer, the Effelsberg 100 m telescope, and the Onsala 25 m telescope. The polarization was linear in PA 0 deg on the sky, and the recording of the signals was carried out with the standard MK II VLBI system with a bandwidth of 2 MHz.

Affiliated with

Also associated with

No associations

Rating

VLBI detection of SS433 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 VLBI detection of SS433, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and VLBI detection of SS433 will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-974056