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Low resolution stellar spectrophotometric observations in the region 1500 Å–3000 Å
Published online by Cambridge University Press: 14 August 2015
Extract
The success of Stecher and Milligan (1962) in obtaining UV photoelectric objective dispersion spectra of stars in 1962 inspired similar work at the Royal Observatory, Edinburgh. For a number of reasons we preferred to build a system using grating dispersion in the convergent beam from a 21-cm diameter paraboloidal mirror (Sudbury, 1969). The same principle of random sky scan from a spinning rocket was employed.
- Type
- Part I: Stellar Fluxes
- Information
- Copyright
- Copyright © Reidel 1970