The origin of the far-ultraviolet continuum in solar and stellar flares

1992 ◽  
Vol 385 ◽  
pp. 731 ◽  
Author(s):  
K. J. H. Phillips ◽  
G. E. Bromage ◽  
J. G. Doyle
1993 ◽  
Vol 419 ◽  
pp. 739 ◽  
Author(s):  
Jayant Murthy ◽  
M. Im ◽  
R. C. Henry ◽  
J. B. Holberg

2011 ◽  
Vol 745 (1) ◽  
pp. 25 ◽  
Author(s):  
Jeffrey L. Linsky ◽  
Rachel Bushinsky ◽  
Tom Ayres ◽  
Juan Fontenla ◽  
Kevin France

2011 ◽  
Vol 196 (2) ◽  
pp. 15 ◽  
Author(s):  
Kwang-Il Seon ◽  
Jerry Edelstein ◽  
Eric Korpela ◽  
Adolf Witt ◽  
Kyoung-Wook Min ◽  
...  

1998 ◽  
Vol 508 (1) ◽  
pp. 370-379 ◽  
Author(s):  
M. Franchini ◽  
C. Morossi ◽  
M. L. Malagnini

2011 ◽  
Vol 734 (1) ◽  
pp. 31 ◽  
Author(s):  
Kevin France ◽  
Eric Schindhelm ◽  
Eric B. Burgh ◽  
Gregory J. Herczeg ◽  
Graham M. Harper ◽  
...  

1989 ◽  
Vol 104 (2) ◽  
pp. 45-48
Author(s):  
K. J. H. Phillips

SummaryUltraviolet continua observed in IUE spectra of dMc stars in a flaring state are compared with those in solar Hares. There is evidence that, as may be the case with solar flares, stellar-flare continua in particularly the λ < 1683 Å region are due to free-bound transitions in neutral silicon excited by ultraviolet lino emission.


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