Low Resolution Spectrum of the Orion Nebula in the 60–300 μ Range
Airborne observations of the Trapezium region of the Orion Nebula in the 60–300 μ range have been made from 13.7 km altitude using a Michelson interferometer with the Rice University 12-in. Flying Infrared Telescope. Fourier analysis of five interferometer scans provided spectra with resolution rang...
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Veröffentlicht in: | Symposium - International Astronomical Union 1973, Vol.52, p.453-457 |
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Format: | Artikel |
Sprache: | eng |
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Zusammenfassung: | Airborne observations of the Trapezium region of the Orion Nebula in the 60–300
μ
range have been made from 13.7 km altitude using a Michelson interferometer with the Rice University 12-in. Flying Infrared Telescope. Fourier analysis of five interferometer scans provided spectra with resolution ranging from 7 cm
–1
to 20 cm
–1
. These spectra were compared with lunar spectra taken with the same instrument at the same altitude to correct for instrumental and atmospheric effects. A weighted combination of these scans provides a low resolution spectrum. The radiation per unit frequency interval at 190
μ
was found to be at least 40% of that measured between 75 and 90
μ.
Neglecting possible features in the spectrum, its general shape is consistent with a blackbody near 70 K. The resolution is inadequate to resolve spectral lines. |
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ISSN: | 0074-1809 |
DOI: | 10.1017/S0074180900054619 |