The Goddard High Resolution Spectrograph: Instrument, goals, and science results

Details The Goddard High Resolution Spectrograph: Instrument, goals, and science results The Goddard High Resolution Spectrograph: Instrument, goals, and science results

Aug 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994pasp..106..890b&link_type=abstract

Astronomical Society of the Pacific, Publications (ISSN 0004-6280), vol. 106, no. 702, p. 890-908

Astronomy and Astrophysics

Astronomy

65

Astronomical Spectroscopy, High Resolution, Interstellar Matter, Spectral Resolution, Stellar Atmospheres, Stellar Evolution, Abundance, Chemical Evolution, Hubble Space Telescope, Mass Transfer, Seyfert Galaxies, Ultraviolet Spectra

Scientific paper

The Goddard High Resolution Spectrograph (GHRS), currently in Earth orbit on the Hubble Space Telescope (HST), operates in the wavelength range 1150-3200 A with spectral resolutions (lambda/delta lambda) of approximately 2 x 103, 2 x 104, and 1 x 103. The instrument and its development from inception, its current status, the approach to operations, representative results in the major areas of the scientific goals, and prospects for the future are described.

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