Radio Observations of Planetary Nebulae

1983 ◽  
pp. 61-68
Author(s):  
P. F. Scott
1981 ◽  
Vol 250 ◽  
pp. 232 ◽  
Author(s):  
S. Kwok ◽  
C. R. Purton ◽  
D. W. Keenan

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.


1971 ◽  
Vol 11 (2) ◽  
pp. 309-321 ◽  
Author(s):  
Joy Heckathorn

1968 ◽  
Vol 34 ◽  
pp. 108-111
Author(s):  
B. Elsmore

Observations have been made of 5 planetary nebulae at 1407 and 408 MHz with beam widths of 23′′ of arc and 80′′ of arc respectively. Measurements of positions, fluxes and angular structure have been obtained; some results are presented in the form of contour maps.


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

2021 ◽  
Vol 919 (2) ◽  
pp. 121
Author(s):  
Marcin Hajduk ◽  
Marijke Haverkorn ◽  
Timothy Shimwell ◽  
Mateusz Olech ◽  
Joseph R. Callingham ◽  
...  

1973 ◽  
Vol 78 ◽  
pp. 875 ◽  
Author(s):  
Yervant Terzian ◽  
John Dickey

1983 ◽  
Vol 103 ◽  
pp. 61-68
Author(s):  
P. F. Scott

A discussion of radio observations for the period up to 1979 forms part of the general review given at the 1979 IAU General Assembly by Terzian (1980) and I shall be concerned here mainly with later results. With the advent of improved radio telescopes and techniques, in particular the coming into full operation of the Very Large Array (VLA), there has been an increasing interest in compact and proto-planetary nebulae and I shall discuss these observations in a separate section of this review.


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