Long-slit spectroscopy in the rocket ultraviolet of the Orion Nebula

Details Long-slit spectroscopy in the rocket ultraviolet of the Orion Nebula Long-slit spectroscopy in the rocket ultraviolet of the Orion Nebula

Jul 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980apj...239..137b&link_type=abstract

Astrophysical Journal, Part 1, vol. 239, July 1, 1980, p. 137-145.

Astronomy and Astrophysics

Astrophysics

14

Abundance, Astronomical Spectroscopy, Emission Spectra, Line Spectra, Nebulae, Ultraviolet Spectrophotometers, Carbon, Data Reduction, Focal Plane Devices, Image Processing, Orion Constellation, Oxygen, Radiative Transfer, Rocket-Borne Instruments, Slits, Spectral Resolution, Spectrographs

Scientific paper

The study deals with the extensive nebulosity in the Trapezium region of Orion. An entrance slit was placed at the focal plane of rocketborne telescope, creating a long-slit spectrograph with a wavelength resolution of 22 A FWHM and a spatial resolution of 14 in. along the slit. Data reduction is outlined, the structure of the Orion Nebula is discussed, and radiative transfer considerations are presented.

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