Showing papers by "Michael W. Werner published in 1974"
TL;DR: In this article, the Owens Valley interferometer was used at 1665, 1667, and 1720 MHz to measure the positions of eleven OH emission sources in W3 (continuum) and NGC 7538.
Abstract: The Owens Valley interferometer was used at 1665, 1667, and 1720 MHz to measure the positions of eleven OH emission sources. The 1720-MHz OH source in W3 (continuum) was found to be 40 seconds away from the H2O maser source and was found not to coincide with any radio or infrared feature. Two OH emission sources were found in NGC 7538; one is identifiable with a very compact radio infrared source, while the other, 80 seconds to the south, is as yet unidentified. The OH sources 0739-14 and Sharpless 269 also coincide with infrared sources.
28 citations
TL;DR: Comet Kohoutek has been observed at wavelengths between 1.25 and 12.5 microns before and after perihelion passage extending to comet-sun distances of 1 AU as mentioned in this paper.
14 citations
TL;DR: The 1-mm continuum flux from Orion Molecular Cloud 2 (OMC-2), measured with a 1-inch beam, is found to be 0.05 plus or minus 0.01 of that from the Becklin-Neugebauer/Kleinmann-Low (BN/KL) complex.
Abstract: The 1-mm continuum flux from Orion Molecular Cloud 2 (OMC-2), measured with a 1-inch beam, is found to be 0.05 plus or minus 0.01 of that from the Becklin-Neugebauer/Kleinmann-Low (BN/KL) complex. This implies that the average density of dust within OMC-2 is about an order of magnitude less than within the BN/KL region.
3 citations