Hostname: page-component-586b7cd67f-g8jcs Total loading time: 0 Render date: 2024-11-30T12:37:39.341Z Has data issue: false hasContentIssue false

A Summary

Published online by Cambridge University Press:  12 April 2016

V. M. Blanco*
Affiliation:
Cerro Tololo Inter-American Observatory

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.

This has been a timely conference. Astronomical spectroscopic classification is facing crossroads that make it wise for us to look carefully at where we are now and which way we should go. The on-going explosion in detection techniques for fainter and fainter objects at all wavelengths and the availability of fast analytical procedures are opening up these new roads. It is a tribute to Fr. Patrick Treanor’s vision that we have gathered here to take stock of the current status and to consider the future of spectral classification and it was fitting that we did so while remembering the pioneering work of Fr. Angelo Secchi

Type
VIII Space Spectroscopy and Future Developments in Classification
Copyright
Copyright © Vatican Observatory 1979