NASA NTRS · 19800054419
Evidence for a variable far-infrared source in NGC 6334
Abstract
NGC 6334 has been mapped with a 40-250 micron photometer with 1 arcmin resolution. Six sources of far-infrared radiation have been detected. The second-strongest source was not detected in an earlier (2.7 years) 40-350 micron survey of the same region. This source is interpreted as a variable far-infrared source. The new source, located at the position of OH and H2O maser sources, is extended (0.7 arcmin FWHM) and has a bolometric luminosity of 190,000 solar luminosities and may represent a hitherto unobserved transient stage of protostellar collapse.
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Mcbreen, B., Fazio, G. G., Stier, M., Wright, E. L.. 1979-09-15. Evidence for a variable far-infrared source in NGC 6334. https://ntrs.nasa.gov/citations/19800054419
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