1977The Astronomical JournalRequires access

Large-beam infrared observations of compact H II regions

II Zeilik M., P. A. Heckert

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Abstract

Near-infrared observations were made of compact H II regions, using a 1.3 m telescope, three infrared photometers, and a large beam (of about one minute). Various techniques were used to calculate the near-infrared extinction, and the corrected flux densities were used to determine 2-25 micron fluxes by fitting the least-squares power law to the points. A mathematical formula and the 4.995-GHz high-resolution radio observations were used to estimate the Lyman-alpha power available to each source. Having corrected for line-of-sight extinction, the 2-25 micron luminosities were found to be approximately equal to or greater than the Lyman-alpha luminosities obtained from radio observations.

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What this paper is about

Near-infrared observations were made of compact H II regions, using a 1.3 m telescope, three infrared photometers, and a large beam (of about one minute). Various techniques were used to calculate the near-infrared extinction, and the corrected flux densities were used to determine 2-25 micron fluxes by fitting the least-squares power law to the points. A mathematical formula and the 4.995-GHz high-resolution radio observations were used to estimate the Lyman-alpha power available to each source. Having corrected for line-of-sight extinction, the 2-25 micron luminosities were found to be approximately equal to or greater than the Lyman-alpha luminosities obtained from radio observations.

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Available abstract

Near-infrared observations were made of compact H II regions, using a 1.3 m telescope, three infrared photometers, and a large beam (of about one minute). Various techniques were used to calculate the near-infrared extinction, and the corrected flux densities were used to determine 2-25 micron fluxes by fitting the least-squares power law to the points. A mathematical formula and the 4.995-GHz high-resolution radio observations were used to estimate the Lyman-alpha power available to each source. Having corrected for line-of-sight extinction, the 2-25 micron luminosities were found to be approximately equal to or greater than the Lyman-alpha luminosities obtained from radio observations.

Key concepts: Physics, Infrared, Astronomy, Astrophysics, Beam (structure), Cosmic infrared background, Optics, Cosmic microwave background

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