The Position of Radio Emission from Nearby Stars

Details The Position of Radio Emission from Nearby Stars The Position of Radio Emission from Nearby Stars

Jun 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983nssl.conf...69j&link_type=abstract

The Nearby Stars and the Stellar Luminosity Function, Proceedings of IAU Colloquium No. 76 held 13-16 June 1983 at Wesleyan Univ

Physics

1

Scientific paper

The position of the radio emission associated with a flare star relative to a background extragalactic radio source has been measured with an accuracy of 0arcsec.01. This emission is probably within 0arcsec.01 of the stellar optical photocenter. Thus the optical reference frame may be related to the radio reference frame at the level of optical accuracy (≡0arcsec.05).

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