Millimeter-VLBI with a Large Millimeter-Array: Future Possibilities
Astrophysics
2007-05-23 v1
Abstract
We discuss possibilities and improvements which could be obtained, if a phased array with a large number (N=50-100) of sub-millimeter antennas - like the planned large southern array (the former LSA, now ALMA) is used for radio-interferometry with very long baselines (VLBI) at millimeter wavelengths. We find that the inclusion of such an instrument in global VLBI network will push the sensitivity and the imaging capabilities of high resolution millimeter interferometry by up to 2 orders of magnitude. This will cause many but todate unforseeable new discoveries.
Keywords
Cite
@article{arxiv.astro-ph/0308044,
title = {Millimeter-VLBI with a Large Millimeter-Array: Future Possibilities},
author = {Thomas P. Krichbaum},
journal= {arXiv preprint arXiv:astro-ph/0308044},
year = {2007}
}
Comments
appeared in: `Science with Large Millimeter Arrays', ESO Astrophysical Symposia, ed. P.A. Shaver, Springer (Berlin Heidelberg), 1996, p. 95-102. 8 pages, 1 figure