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Bitmap Image  |  1995-11-13  |  12KB  |  193x384  |  1-bit (2 colors)
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OCR: ong hot central stars that er ultraviolet radiation radiation is in turm hs ghtl particles which then (this process is known fluorescence) two The body ofM27 COr his opposing dark areas b1 181 image) and two broad ause lobes joined a.t the cent of this structure the ne the given its more popular Durmbbell Nebula uite The Durnbbell Nebu ich ir close to our solar syster part explains why thei shows such intricate expanding shell and br cloud well -defined edges of t are clearly visible radiatior ightly fluor Ftwo ioined popula Durbbell syste panding sheli