scholarly journals Simulations of a Population of Planetary Nebulae

1993 ◽  
Vol 155 ◽  
pp. 461-464
Author(s):  
G. Stasinska ◽  
R. Tylenda

We present a simulation of the population of Galactic bulge planetary nebulae (GBPN), which matches the diagrams obtained from VLA radio observations. This simulation may not be the only one fitting the observed data, but it helps understanding the role of observational uncertainties and selection effects in the interpretation of observational diagrams.

2001 ◽  
Vol 373 (2) ◽  
pp. 536-541 ◽  
Author(s):  
G. C. Van de Steene ◽  
G. H. Jacoby

2011 ◽  
Vol 7 (S283) ◽  
pp. 380-381
Author(s):  
Marcin Hajduk ◽  
Albert A. Zijlstra

AbstractWe present new observations in the radio continuum of 31 planetary nebulae at 5 and 8 GHz with the Australian Telescope Compact Array. The observations are used to invesigate properties of the interstellar extinction toward Galactic Bulge.


2017 ◽  
Vol 422 (1-2) ◽  
pp. 479-493 ◽  
Author(s):  
Xiao-Fei Li ◽  
Cheng-Bao Wang ◽  
Wei-Ping Zhang ◽  
Le-Hua Wang ◽  
Xiu-Li Tian ◽  
...  

2009 ◽  
Vol 5 (S265) ◽  
pp. 354-355
Author(s):  
Oscar Cavichia ◽  
Roberto D. D. Costa ◽  
Walter J. Maciel

AbstractNew abundances of planetary nebulae located towards the bulge of the Galaxy are derived based on observations made at LNA (Brazil). We present accurate abundances of the elements He, N, S, O, Ar, and Ne for 56 PNe located towards the galactic bulge. The data shows a good agreement with other results in the literature, in the sense that the distribution of the abundances is similar to those works. From the statistical analysis performed, we can suggest a bulge-disk interface at 2.2 kpc for the intermediate mass population, marking therefore the outer border of the bulge and inner border of the disk.


Author(s):  
G. Stasinska ◽  
A. Acker ◽  
A. Fresneau ◽  
J. F. Gameiro ◽  
J. Köppen ◽  
...  

1989 ◽  
pp. 167-167
Author(s):  
M. W. Feast ◽  
T. D. Kinman ◽  
B. S. Lasker

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