More high-quality observations of stellar spectra.

Details More high-quality observations of stellar spectra. More high-quality observations of stellar spectra.

Mar 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979msngr..16...20h&link_type=abstract

The Messenger, vol. 16, p. 20-20

Astronomy and Astrophysics

Astrophysics

Spectrophotometry:Spectrum Variables

Scientific paper

With its large light-gathering power, the VLT will permit spectra of even rather faint objects to be obtained with short exposure times. It will therefore become possible to observe rapid changes in, for instance, the emission lines in nova spectra and to learn about the physical conditions of a nova outburst. Professor Uw Houziaux of the Astrophysical Institute in Liege, Belgium, expects to observe spectrally variable stars with the VLT and also to do very accurate spectrophotometry of a number of brighter stars.

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