Discovery of a fast radiative shock wave in the Cygnus Loop using the Hopkins Ultraviolet Telescope

1991 ◽  
Vol 379 ◽  
pp. L33 ◽  
Author(s):  
William P. Blair ◽  
Knox S. Long ◽  
Olaf Vancura ◽  
Charles W. Bowers ◽  
Arthur F. Davidsen ◽  
...  
1983 ◽  
Vol 275 ◽  
pp. 636 ◽  
Author(s):  
J. C. Raymond ◽  
W. P. Blair ◽  
R. A. Fesen ◽  
T. R. Gull

1985 ◽  
Vol 297 ◽  
pp. 476 ◽  
Author(s):  
L. Binette ◽  
M. A. Dopita ◽  
I. R. Tuohy

2015 ◽  
Vol 814 (2) ◽  
pp. 165 ◽  
Author(s):  
John C. Raymond ◽  
Richard J. Edgar ◽  
P. Ghavamian ◽  
William P. Blair
Keyword(s):  

2015 ◽  
Vol 805 (2) ◽  
pp. 152 ◽  
Author(s):  
John C. Raymond ◽  
Richard J. Edgar ◽  
Parviz Ghavamian ◽  
William P. Blair
Keyword(s):  

2013 ◽  
Vol 9 (S296) ◽  
pp. 160-164 ◽  
Author(s):  
Ravi Sankrit ◽  
William P. Blair ◽  
John C. Raymond ◽  
Brian J. Williams

AbstractThe Cygnus Loop supernova remnant serves as an excellent laboratory for the study of radiative and non-radiative shocks with speeds in the 150–450 km s−1 range. We present results on shock-excited emission and dust destruction based on Spitzer Space Telescope observations of two well-studied regions in the remnant, (i) a non-radiative shock filament along the NE limb, and (ii) the XA region, characterized by emission from bright radiative shocks.


1984 ◽  
Vol 276 ◽  
pp. 653 ◽  
Author(s):  
M. A. Dopita ◽  
L. Binette ◽  
S. Dodorico ◽  
P. Benvenuti

1992 ◽  
Vol 190 (2) ◽  
pp. 169-176
Author(s):  
V. K. Singh ◽  
Kishor Kumar Srivastava

2003 ◽  
Vol 584 (2) ◽  
pp. 770-781 ◽  
Author(s):  
John C. Raymond ◽  
Parviz Ghavamian ◽  
Ravi Sankrit ◽  
William P. Blair ◽  
Salvador Curiel

2001 ◽  
Vol 560 (2) ◽  
pp. 763-771 ◽  
Author(s):  
J. C. Raymond ◽  
J. Li ◽  
William P. Blair ◽  
Robert H. Cornett
Keyword(s):  

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