𝔖 Bobbio Scriptorium
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The spectra of novae

✍ Scribed by Dean B. McLaughlin

Publisher
Elsevier Science
Year
1956
Tongue
English
Weight
835 KB
Volume
2
Category
Article
ISSN
0083-6656

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πŸ“œ SIMILAR VOLUMES

Expanding atmosphere models for SSS spec
Expanding atmosphere models for SSS spectra of novae
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## Abstract Super Soft Source (SSS) spectra are powered by nuclear burning on the surface of a white dwarf. The released energy causes a radiatively‐driven wind that leads to a radially extended atmosphere around the white dwarf. Significant blue shifts in photospheric absorption lines are found in

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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

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