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Low Frequency (327 MHz) VLBI Survey: First Results

  • V. Altunin (a1), A. Beasley (a2), E. Lűdke (a3), V. Alekseev (a4), B. Lipatov (a4), R. Dagkesamansky (a5), N. Kardashev (a5), A. Kovalenko (a5), I. Molotov (a5), V. Slysh (a5) and V. Migenes (a6)...

Abstract

In this paper we report the first results of the 327 MHz VLBI survey which has been carried out in the last two years to select potential candidate sources for the future SVLBI missions and to search for directions of small scattering-“holes” in the interstellar scattering medium. During the three VLBI sessions conducted so far, we observed about 80 sources. Preliminary data analyzed from the first part of the survey shows that at least 17 out of 50 sources have compact components with a size smaller than 30 mas.

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Copyright

References

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Johnston, K.L., et al. 1995. AJ, 110, 880920.
Polatidis, A.G., et al. 1995. ApJS, 98, 132.

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