Ionization structure and composition of the planetary nebula NGC 7027

1978 ◽  
Vol 219 ◽  
pp. 565 ◽  
Author(s):  
G. A. Shields
2020 ◽  
Vol 898 (1) ◽  
pp. 86
Author(s):  
R. C. Forrey ◽  
J. F. Babb ◽  
E. D. S. Courtney ◽  
R. T. McArdle ◽  
P. C. Stancil
Keyword(s):  

2011 ◽  
Vol 7 (S283) ◽  
pp. 340-341 ◽  
Author(s):  
Ashkbiz Danehkar ◽  
David J. Frew ◽  
Quentin A. Parker ◽  
Orsola De Marco

AbstractWe estimate distances to the spherical planetary nebula Abell 39 and the bipolar planetary nebula NGC 7027 by interpolating from a wide grid of photoionization models using the 3-D code, MOCASSIN. We find preliminary distances of 1.5 kpc and 0.9 kpc respectively, with uncertainties of about 30%.


2001 ◽  
Vol 550 (2) ◽  
pp. L189-L192 ◽  
Author(s):  
Joel H. Kastner ◽  
Saeqa D. Vrtilek ◽  
Noam Soker
Keyword(s):  
X Ray ◽  

1954 ◽  
Vol 120 ◽  
pp. 401 ◽  
Author(s):  
Lawrence H. Aller
Keyword(s):  

1976 ◽  
Vol 209 ◽  
pp. 793 ◽  
Author(s):  
R. R. Treffers ◽  
U. Fink ◽  
H. P. Larson ◽  
T. N., III Gautier
Keyword(s):  

1993 ◽  
Vol 105 ◽  
pp. 250 ◽  
Author(s):  
James R. Graham ◽  
E. Serabyn ◽  
T. M. Herbst ◽  
K. Matthews ◽  
G. Neugebauer ◽  
...  

1978 ◽  
Vol 76 ◽  
pp. 162-162
Author(s):  
Daniel Péquignot

It is demonstrated that ionization structure of NGC 7027 cannot be explained by static models based on the standard photoionization theory unless some complementary physical process is included. The main discrepancies are successfully eliminated by including charge transfer reactions with hydrogen for the following ions: C+, C+3, N+2, O+2, Ne+2, S+ and S+3, the rate coefficients being probably of the order of or larger than 10−9cm+3s−1 except for C+ and Ne+2; in addition the charge exchange rate for N+ is probably ∼200 times smaller than the value proposed by Steigman et al. (1971).


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