Conformationally restrained degenerate base analogues

1993 ◽  
Vol 58 (s1) ◽  
pp. 41-43
Author(s):  
D. M. Williams ◽  
Daniel M. Brown
2002 ◽  
Vol 12 (24) ◽  
pp. 3641-3643 ◽  
Author(s):  
Akimitsu Okamoto ◽  
Kazuo Tanaka ◽  
Isao Saito

2018 ◽  
Vol 86 (10) ◽  
pp. 1111-1116
Author(s):  
Rebecca Vera ◽  
Melissa Synsmir-Zizzamia ◽  
Sarah Ojinnaka ◽  
David A. Snyder

1979 ◽  
Vol 53 ◽  
pp. 290-293
Author(s):  
G. Siegfried Kutter ◽  
Warren M. Sparks

We assume that the outburst of classical novae is the result of transfer of H-rich material from a red secondary star to a He or C/O white dwarf and the development of a thermonuclear runaway in the e-degenerate “base of the accreted H-rich envelope. Based on these assumptions, we have investigated this problem in several stages of increasing theoretical complexity and physical realism.


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