scholarly journals The illumination of the cometary nebula 1548C27

1991 ◽  
Vol 249 (2) ◽  
pp. 310-312 ◽  
Author(s):  
S. M. Scarrott ◽  
C. D. Rolph ◽  
C. N. Tadhunter
Keyword(s):  
1987 ◽  
Vol 115 ◽  
pp. 191-192
Author(s):  
Yervant Terzian ◽  
Kenneth C. Turner

We have performed high resolution VLA radio observations for several small H II regions, including the cluster emission nebulae S258, S255, S257, and S256. The region (PP56) between S255 and S257 at λ2 cm reveals significant flux structure close to OH, H2O and infrared emitting sources as shown in Figure 1. The flux densities and positions are indicated in Table 1. Observations of the cometary nebula PP59 (S269) also reveal similar characteristics as shown in Figure 2. These regions are considered to be active star-forming clouds. The cometary nebula PP40 was also observed and we note that its physical parameters are very similar to those of a typical planetary nebula.


1978 ◽  
Vol 226 ◽  
pp. 455
Author(s):  
T. T. Arny ◽  
K. P. Bechis
Keyword(s):  

Astrophysics ◽  
1979 ◽  
Vol 14 (3) ◽  
pp. 289-291 ◽  
Author(s):  
�. S. Parsamyan ◽  
V. M. Petrosyan
Keyword(s):  

1994 ◽  
Vol 268 (1) ◽  
pp. L60-L62
Author(s):  
S. M. Scarrott ◽  
D. P. Stockdale ◽  
P. W. Draper

Astrophysics ◽  
1967 ◽  
Vol 1 (4) ◽  
pp. 221-227 ◽  
Author(s):  
E. E. Khachikyan ◽  
E. S. Parsamyan
Keyword(s):  

1982 ◽  
Vol 198 (4) ◽  
pp. 881-888 ◽  
Author(s):  
M. R. Gething ◽  
R. F. Warren-Smith ◽  
S. M. Scarrott ◽  
R. G. Bingham

Astrophysics ◽  
1974 ◽  
Vol 8 (1) ◽  
pp. 8-16
Author(s):  
M. A. Kazaryan ◽  
�. E. Khachikyan

1987 ◽  
pp. 188-188
Author(s):  
M. Tapia ◽  
M. Roth ◽  
L. F. Rodríguez ◽  
J. Cantó ◽  
P. Persi ◽  
...  

1977 ◽  
Vol 215 ◽  
pp. L127 ◽  
Author(s):  
M. Cohen ◽  
L. V. Kuhi ◽  
E. A. Harlan

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