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Observational evidence for the two types of dwarf nova outbursts

✍ Scribed by J. Smak


Publisher
Springer Netherlands
Year
1987
Tongue
English
Weight
188 KB
Volume
131
Category
Article
ISSN
0004-640X

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## Abstract For several novae, a bright X‐ray source with a spectrum resembling the class of Super Soft X‐ray Sources (SSS) has been observed a few weeks to months after outburst. Novae are powered by explosive nuclear burning on the surface of a white dwarf, and enough energy is produced to power