Near-Infrared Spectroscopy of V1974 Cygni 1992: New Coronal Emission Lines in Classical Novae

1996 ◽  
Vol 467 ◽  
pp. 860 ◽  
Author(s):  
R. Mark Wagner ◽  
D. L. Depoy
2003 ◽  
Vol 209 ◽  
pp. 269-270
Author(s):  
Douglas M. Kelly ◽  
Bruce J. Hrivnak

We measured 2.1 – 2.3 μm spectra for a fairly complete sample of known proto-planetary nebulae (PPN) at declinations greater than -30°. This spectral range includes the H2 emission lines 1-0 S(1), 1-0 S(0), 2-1 S(1), 2-1 S(2), and 3-2 S(3). We detected H2 emission from 16 of the 51 nebulae in our survey, including radiatively-excited H2 from several non-bipolar PPN.


1990 ◽  
Vol 100 ◽  
pp. 1588 ◽  
Author(s):  
Robert A. Benjamin ◽  
Harriet L. Dinerstein

2012 ◽  
Vol 760 (2) ◽  
pp. 153 ◽  
Author(s):  
Joseph P. Liskowsky ◽  
Sean D. Brittain ◽  
Joan R. Najita ◽  
John S. Carr ◽  
Greg W. Doppmann ◽  
...  

2013 ◽  
Vol 767 (2) ◽  
pp. 159 ◽  
Author(s):  
Sean D. Brittain ◽  
Joan R. Najita ◽  
John S. Carr ◽  
Joseph Liskowsky ◽  
Matthew R. Troutman ◽  
...  

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