Hostname: page-component-7bb8b95d7b-cx56b Total loading time: 0 Render date: 2024-09-27T01:44:07.191Z Has data issue: false hasContentIssue false
  • English
  • Français

Future Spectral Line Research with the VLA

Published online by Cambridge University Press:  14 August 2015

K. J. Johnston
K. J. Johnston*
Affiliation:
E.O. Hulbert Center for Space Research, Naval Research Laboratory, Washington, D.C. 20375

Extract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

The Very Large Array (VLA) is presently being constructed on the Plains of San Augustine near Socorro, New Mexico by the National Radio Astronomy Observatory. The purpose for which this instrument is being constructed is to produce “radio images” of resolution comparable to that of large optical telescopes. There have already been several “test” observations, some successful, using the partially completed instrument to study the molecular species of OH, H2O, and NH3 with wide bandwidths (200-1500 kHz).

Type
Research Article
Information
Symposium - International Astronomical Union , Volume 87: Interstellar Molecules , 1980 , pp. 627 - 629
Copyright
Copyright © Reidel 1980