A Hot Spot Model for GR Tauri

Author(s):  
B. Soonthornthum ◽  
A. Aungwerojwit ◽  
Y. Yang ◽  
Q. Liu
Keyword(s):  
Hot Spot ◽  
2021 ◽  
Vol 215 ◽  
pp. 103544
Author(s):  
Zhaoxia Jiang ◽  
Sanzhong Li ◽  
Qingsong Liu ◽  
Jianli Zhang ◽  
Zaizheng Zhou ◽  
...  
Keyword(s):  
Hot Spot ◽  

JETP Letters ◽  
2018 ◽  
Vol 108 (4) ◽  
pp. 270-278 ◽  
Author(s):  
V. L. Vadimov ◽  
D. Yu. Vodolazov ◽  
S. V. Mironov ◽  
A. S. Mel’nikov

1979 ◽  
Vol 3 (5) ◽  
pp. 311-312 ◽  
Author(s):  
D. T. Wickramasinghe ◽  
N. Visvanathan

Since the discovery of variable circular and linear polarisation in VV Puppis (Tapia 1977), several investigators have observed the system. The new observations particularly of polarisation (Liebert et al. 1978, Liebert and Stockman 1979 have ruled out the standard dwarf nova (accretion disc — hot spot) model previously used to interpret the light curve of VV Puppis.


2004 ◽  
Vol 98 (4) ◽  
pp. 748-759 ◽  
Author(s):  
É. Z. Kuchinskii ◽  
M. V. Sadovskii ◽  
N. A. Strigina

2015 ◽  
Vol 92 (7) ◽  
Author(s):  
Vanuildo S. de Carvalho ◽  
Thomas Kloss ◽  
Xavier Montiel ◽  
Hermann Freire ◽  
Catherine Pépin

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