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Fe XIII line in R Aquarii (1976)

Zirin, H.

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Publication Date: 2011-08-16

Description: The emission line of the forbidden coronal transition of Fe XIII at 10,747 A has been detected in data from a spectral survey at R Aquarii. Strong emission lines of He I at 10,830 A and P gamma have been identified; a line at 11,013 A may be He I 3(1)S-6(1)P. It is suggested that the observed iron line is produced by a corona surrounding R Aquarii inter alia. The corona may be the source of the radio emission reported by Gregory and Seaquist (1974).

Keywords: ASTROPHYSICS

Type: Nature; 259; Feb. 12

Format: text

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