Concurrent 43 and 86 GHz VLBA Polarimetry Observations of the Quasars 3C 273 and 3C 279

Details Concurrent 43 and 86 GHz VLBA Polarimetry Observations of the Quasars 3C 273 and 3C 279 Concurrent 43 and 86 GHz VLBA Polarimetry Observations of the Quasars 3C 273 and 3C 279

Dec 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005aspc..340..171a&link_type=abstract

Future Directions in High Resolution Astronomy: The 10th Anniversary of the VLBA, ASP Conference Proceedings, Vol. 340. Edited

Astronomy and Astrophysics

Astronomy

1

Scientific paper

Here we present new 43 and 86 GHz VLBA observations of the 3C 273 and 3C
279 collected concurrently in May 2002. These observations confirm prior
86 GHz CMVA results from April 2000. An observed differential Faraday
rotation in 3C 273 implies a Faraday screen of at least 29000 rad
m-2 is present ˜0.9 mas from the core.

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