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At least 883 records · Page 49
All sourcesNASA NTRSDOE OSTI
NASA NTRS1974

A high-resolution map of the Orion Nebula region at far-infrared wavelengths

It is shown that the Kleinmann-Low nebula continues to radiate like a 70-deg-K blackbody at 69 microns, as it does at shorter wavelengths, but that most of the 69-micron flux from Ori A (M42) comes from an extended emission that roughly follows the free-free radio emission. Nearby sources also detected include the nebula M43 and the molecular cloud OMC-2.

Fazio, G. G.↗
NASA NTRS1975

Ultraviolet spectrophotometry from Gemini 11 of stars in Orion

Ultraviolet spectrophotometry in the wavelength region 2600-3600 A is reported for the bright early-type stars beta, eta, gamma, delta, iota, epsilon, sigma, zeta, and kappa Ori. The results are in good agreement with other observations, and, with the possible exception of the supergiants, are in good agreement with recent line-blanketed model atmospheres. There is evidence that the supergiants possess a small ultraviolet deficiency shortward of 3000 A relative to main-sequence stars of similar spectral type. The most extreme example of this phenomenon is the star kappa Ori.

Morgan, T. H.↗
NASA NTRS1978

Far infrared polarization of the Kleinmann-Low Nebula in Orion

Elongated dust grains aligned by local magnetic fields are though to absorb background radiation and produce linear and circular polarization which exhibit strong wavelength dependence in the near infrared. The NASA Kuiper observatory 91 cm infrared telescope was used to observe polarization characteristics of the Kleinmann-Low nebula in four far infrared wavelength bands in order to detect emission from these same oriented grains at longer wavelengths, and determine whether this radiation shows a direction of polarization perpendicular to that seen in the near infrared. The polarization, if any, that characterized the radiation in the three longest wavelength filter positions (28-48 micron, 44-72 micron, and 70-115 micron) is small. The noisiest measurements were obtained in the 16-33 micron filter position. Possible explanations for the low polarization observed at long wavelengths are explored.

Gull, G. E.↗
NASA NTRS1978

Lamellar grating observations of the Orion Nebula from 100 to 500 microns

Results are presented for spectroscopic observations of the Kleinmann-Low nebula in the 100-500-micron region taken from the Kupier Airborne Observatory. These results, in conjunction with previous work at shorter wavelengths, are consistent with a dilute blackbody spectrum modified by grain emissivity and spatial variations in the grain density.

Pipher, J. L.↗
NASA NTRS1978

Far-infrared polarization of the Kleinmann-Low Nebula in Orion

Polarization observed in the Kleinmann-Low Nebula is described. The observations were obtained by the Kuiper Airborne Observatory at an altitude of 12 km and in wavelength ranges 16-26, 28-48, 44-72, and 71-115 microns. Beyond 28 microns, the 2% polarization detected is consistent with zero polarization, while the upper limit in the 16-26 micron range is 7% polarization. It is suggested that the smallness of the detected polarization restricts nebula models for explaining the observations.

Gull, G. E.↗
NASA NTRS1981

A frequency and timing subsystem for the ORION mobile unit

A mobile surveying instrument in support of the crustal dynamics program measures the length and direction of the distance between sites on the Earth's surface using VLBI techniques operating at microwave frequencies and extragalactic radio sources. The frequency and timing subsystem uses as a frequency standard the hydrogen maser. An important part of the subsystem is a sophisticated automatic system to monitor frequency stability and accumulated clock error.

Clements, P. A.↗