Continuum Formation
Continuum Formation is a radiative process in stellar atmospheres that belongs to the class of spectral formation mechanisms, specifically distinguished by the production of a smooth, continuous spectrum arising from the collective effects of bound-free, free-free, and free-bound transitions in ionized gases, rather than from discrete atomic line emissions.
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10.9K
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854
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325
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Supercontinuum Generation in Gases
P. B. Corkum, C. Rolland, T. Srinivasan-Rao · Physical Review Letters · 1986 · 405 citations
Electron spectra from multiphoton ionization of xenon at 1064, 532, and 355 nm
P. Kruit, J. Kimman, H. G. Muller et al. · Physical review. A, General physics · 1983 · 386 citations
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Goddard Space Flight Center
Greenbelt, United States
13 h-index
36 publications
1.9K citations
Center for Astrophysics Harvard & Smithsonian
Cambridge, United States
10 h-index
30 publications
1.6K citations

University of Leicester
Leicester, United Kingdom
9 h-index
20 publications
1.2K citations
University of Cambridge
Cambridge, United Kingdom
8 h-index
22 publications
875 citations
Nicolaus Copernicus Astronomical Center
Warsaw, Poland
8 h-index
12 publications
573 citations
California Institute of Technology
Pasadena, United States
7 h-index
14 publications
672 citations
Queen's University Belfast
Belfast, United Kingdom
6 h-index
28 publications
900 citations
Institute of Astronomy
Moscow, Russia
5 h-index
6 publications
251 citations
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ApJ · 49 publications · 3.7K citations
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38 publications · 1.9K citations
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16 publications · 789 citations
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AJ · 5 publications · 248 citations
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