Theoretical emission line strengths for Ne VII compared to EUV solar observations

Solar Physics ◽  
1991 ◽  
Vol 131 (2) ◽  
pp. 291-296 ◽  
Author(s):  
F. P. Keenan
Keyword(s):  
Emission Line ◽  
Solar Observations ◽  
Line Strengths

Theoretical emission line strengths for Ov compared to EUV solar observations

Solar Physics ◽  
1994 ◽  
Vol 150 (1-2) ◽  
pp. 61-70 ◽  
Author(s):  
F. P. Keenan ◽  
G. A. Warren ◽  
J. G. Doyle ◽  
K. A. Berrington ◽  
A. E. Kingston
Keyword(s):  
Emission Line ◽  
Solar Observations ◽  
Line Strengths

Relative quasar luminosities determined from emission line strengths

Nature ◽  
1978 ◽  
Vol 273 (5662) ◽  
pp. 431-435 ◽  
Author(s):  
Jack A. Baldwin ◽  
William L. Burke ◽  
C. Martin Gaskell ◽  
E. J. Wampler
Keyword(s):  
Emission Line ◽  
Line Strengths

Is there a Relation between Optical Emission Line Strengths and Continuum Shapes?

1989 ◽  
pp. 187-188
Author(s):  
Belinda J. Wilkes ◽  
Martin Elvis ◽  
Jonathan McDowell
Keyword(s):  
Emission Line ◽  
Optical Emission ◽  
Line Strengths

AL II emission-line strengths in low-density astrophysical plasmas

1992 ◽  
Vol 385 ◽  
pp. 375 ◽  
Author(s):  
F. P. Keenan ◽  
L. K. Harra ◽  
K. M. Aggarwal ◽  
W. A. Feibelman
Keyword(s):  
Emission Line ◽  
Low Density ◽  
Astrophysical Plasmas ◽  
Line Strengths

scholarly journals New Models for Massive Star Populations in Young Starbursts: Summary of the Models and Applications

1999 ◽  
Vol 186 ◽  
pp. 285-285
Author(s):  
Daniel Schaerer ◽  
William D. Vacca
Keyword(s):  
Emission Line ◽  
Stellar Evolution ◽  
Massive Star ◽  
Optical Emission ◽  
Emission Lines ◽  
Evolutionary Synthesis ◽  
Stellar Spectra ◽  
New Models ◽  
Helium Emission ◽  
Line Strengths

Using the latest stellar evolution models, theoretical stellar spectra, and a compilation of observed emission line strengths from Wolf-Rayet (WR) stars, we have constructed evolutionary synthesis models for young starbursts (Schaerer & Vacca 1997; see also Schaerer 1996). We provide detailed predictions of UV and optical emission line strengths for both the WR stellar lines and the major nebular hydrogen and helium emission lines, as a function of several input parameters related to the starburst episode.

Variation of Emission-Line Strengths across M31

1972 ◽  
Vol 177 ◽  
pp. 31 ◽  
Author(s):  
Vera C. Rubin ◽  
C. Krishna Kumar ◽  
W. Kent, Jr. Ford
Keyword(s):  
Emission Line ◽  
Line Strengths
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