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AbstractAbstract
[en] The distributions of energy in the ultraviolet continuum (λλ 1500-3500 A) of three diffuse nebulae (NGC 1976, NGC 6523 and NGC 6618) and two planetary nebulae (NGC 6853 and NGC 2392) are presented. For the planetary nebulae, the radiation fluxes in the brightest emission lines are determined
Original Title
Nablyudeniya diffuznykh i planetarnykh tumannostej na astrofizicheskoj stantsii Astron
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For English translation see the journal Soviet Astronomy (USA).
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Journal Article
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