The problem of star formation - and what ten nights of sub-millimetre observations with the VLT could contribute to its solution.

Details The problem of star formation - and what ten nights of sub-millimetre observations with the VLT could contribute to its solution. The problem of star formation - and what ten nights of sub-millimetre observations with the VLT could contribute to its solution.

Jun 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979msngr..17...15m&link_type=abstract

The Messenger, vol. 17, p. 15-18

Astronomy and Astrophysics

Astronomy

Star Formation

Scientific paper

Astronomical observations are regularly carried out over the whole electromagnetic spectrum, from y-rays to low-frequency radio waves. There are few unexplored "holes", but one of these-in the neighbourhood of 1 mm-is exactly where we expect most of the radiation from stars during their early stages of formation. The VL T would be ideally suited for ground-based observations in the sub-millimetre range, because of its large surface and good angular resolution. Dr. Peter Mezger of the Max Planck Institute for Radioastronomy in Bonn explains how the VL T can make a very important contribution to the study of stellar formation.

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