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2014 ◽  
Vol 40 (6) ◽  
pp. 343-352
Author(s):  
S. O. Medzhidova ◽  
Kh. M. Mikailov ◽  
B. N. Rustamov
Keyword(s):  

2014 ◽  
Vol 30 (2) ◽  
pp. 85-91
Author(s):  
S. O. Mejidova ◽  
B. N. Rustamov ◽  
Kh. M. Mikayilov ◽  
I. A. Alekberov
Keyword(s):  

Astrophysics ◽  
2012 ◽  
Vol 55 (2) ◽  
pp. 147-155 ◽  
Author(s):  
A. N. Rostopchina-Shakhovskaja ◽  
V. P. Grinin ◽  
D. N. Shakhovskoi
Keyword(s):  

2012 ◽  
Vol 56 (5) ◽  
pp. 379-394 ◽  
Author(s):  
V. I. Shenavrin ◽  
V. P. Grinin ◽  
A. N. Rostopchina-Shakhovskaja ◽  
T. V. Demidova ◽  
D. N. Shakhovskoi
Keyword(s):  
Cq Tau ◽  

Astrophysics ◽  
2006 ◽  
Vol 49 (2) ◽  
pp. 151-163 ◽  
Author(s):  
O. V. Kozlova ◽  
D. N. Shakhovskoi ◽  
A. N. Rostopchina ◽  
I. Yu. Alekseev
Keyword(s):  

2001 ◽  
Vol 27 (6) ◽  
pp. 376-378
Author(s):  
D. N. Shakhovskoi ◽  
O. S. Shulov ◽  
E. N. Kopatskaya
Keyword(s):  

1998 ◽  
Vol 15 (1-4) ◽  
pp. 159-163 ◽  
Author(s):  
A. N. Rostopchina ◽  
V. P. Grinin ◽  
D. N. Shakhovskoy ◽  
P. S. Thé

1994 ◽  
Vol 162 ◽  
pp. 392-393
Author(s):  
N.V. Voshchinnikov ◽  
V.B. Il'in ◽  
A.F. Kholtygin

Herbig Ae/Be (HAEBE) stars are young objects with strong infrared excesses, variable brightness, intrinsic polarization and complex spectral line profiles. Almost all of these features are due to the presence of circumstellar (CS) shells. We consider the group of HAEBE stars with non-periodic Algol-like minima (UX Ori, WW Vul, etc.). They have irregular brightness drops by 2–3 mag in the visual, accompanied by an increase of linear polarization.


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