Radio source structure and VLBI position instabilities - Archive ouverte HAL
Communication Dans Un Congrès Année : 2013

Radio source structure and VLBI position instabilities

Romuald Bouffet
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P. Charlot
S. Lambert
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Résumé

Astrometric positions of extragalactic radio sources derived from VLBI data are used to build highly-accurate reference frames such as the International Celestial Reference Frame. Despite their distant locations, instabilities in the position of these sources are often seen on time scales of months to years, which is generally thought to be caused by source structure evolution. In this paper, we compare position instabilities and structural evolution for a sample of 68 sources observed over a 10-year period (1994--2003). Our results indicate that the two phenomena are linked at some level although the correlation is not perfect.
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Dates et versions

hal-00909556 , version 1 (26-11-2013)

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Romuald Bouffet, P. Charlot, S. Lambert. Radio source structure and VLBI position instabilities. Proceedings SF2A 2013 - Scientific highlights, Montpellier : France (2013), 2013, Montpellier, France. pp.161-164. ⟨hal-00909556⟩

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