Absorption of 3.5-m. Radiation in the Optical Emission Nebula, NGC 6357

Details Absorption of 3.5-m. Radiation in the Optical Emission Nebula, NGC 6357 Absorption of 3.5-m. Radiation in the Optical Emission Nebula, NGC 6357

Jan 1956

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1956natur.177..178m&link_type=abstract

Nature, Volume 177, Issue 4500, pp. 178 (1956).

Computer Science

2

Scientific paper

IN the course of a radio survey of bright emission nebulæ with the 1,500-ft. Sydney cross-aerial, some fourteen nebulæ were studied at a wave-length of 3.5 m. Six were probably observed in emission, seven were undetectable, and one, NGC 6357, was observed in absorption. The observation of NGC 6357 is the first reported case of absorption of radio waves by an emission nebula ; it leads to an estimate of the electron temperature of the nebula based almost entirely on radio data. In this preliminary communication the observation and its consequences are discussed briefly ; a more complete account of the survey will be given elsewhere.

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