Analysis of ghost spectra which simulate the absorption-line spectrum of 4C 05.34

1975 ◽  
Vol 201 ◽  
pp. 547 ◽  
Author(s):  
Y. P. Varshni
1973 ◽  
Vol 183 ◽  
pp. 767 ◽  
Author(s):  
P. A. Strittmatter ◽  
R. F. Carswell ◽  
E. M. Burbidge ◽  
C. Hazard ◽  
J. A. Baldwin ◽  
...  

1977 ◽  
Vol 216 ◽  
pp. 351 ◽  
Author(s):  
R. F. Carswell ◽  
M. G. Smith ◽  
J. A. J. Whelan

2013 ◽  
Vol 37 (1) ◽  
pp. 17-27 ◽  
Author(s):  
Ji Tuo ◽  
Zhou Hong-yan ◽  
Wang Ting-gui ◽  
Wang Hui-yuan

1974 ◽  
Vol 189 ◽  
pp. 195 ◽  
Author(s):  
K. S. Anderson

1976 ◽  
Vol 205 ◽  
pp. L117 ◽  
Author(s):  
E. M. Burbidge ◽  
R. D. Caldwell ◽  
H. E. Smith ◽  
J. Liebert ◽  
H. Spinrad
Keyword(s):  

2010 ◽  
Vol 6 (S272) ◽  
pp. 610-611
Author(s):  
Vitaly P. Goranskij ◽  
Elena Bersukova

AbstractCCD photometry reveals a hot spot on the surface of the hot accretion gainer in this supergiant O type binary with a big accretion rate. This spot is as bright as 25000 Suns. The orbital period of this system is 33.108 days. The absorption-line spectrum contains multiple lines of He I, Si III and N II. The star is associated with H II region formed by bipolar gas outflow from the system.


2002 ◽  
Vol 44 (11) ◽  
pp. 2204-2209 ◽  
Author(s):  
B. S. Razbirin ◽  
A. N. Starukhin ◽  
A. V. Chugreev ◽  
A. S. Zgoda ◽  
V. P. Smirnov ◽  
...  

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