X-ray emission from the ring nebula NGC6888

Details X-ray emission from the ring nebula NGC6888 X-ray emission from the ring nebula NGC6888

Apr 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988natur.332..518b&link_type=abstract

Nature (ISSN 0028-0836), vol. 332, April 7, 1988, p. 518-520.

Computer Science

59

Nebulae, Stellar Winds, Wolf-Rayet Stars, X Ray Sources, Interstellar Gas, Interstellar Matter, Stellar Envelopes

Scientific paper

Soft X-ray emission from the ring nebula NGC 6888, formed by the stellar wind of the central Wolf-Rayet star HD 192163, has been found after thorough processing of Einstein observation data. A new class of X-ray sources, predicted some 20 years ago, has thus been discovered. The spectral shape agrees completely with theoretical predictions, but the emission flux is more than an order of magnitude less than the predictions.

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