scholarly journals Two‐dimensional Photometric Decomposition of the TeV BL Lacertae Objects Markarian 421, Markarian 501, and 1ES 2344+514

1999 ◽  
Vol 111 (764) ◽  
pp. 1223-1232 ◽  
Author(s):  
 K. Nilsson ◽  
T. Pursimo ◽  
L. O. Takalo ◽  
A. Sillanpää ◽  
H. Pietilä ◽  
...  
1978 ◽  
Vol 224 ◽  
pp. 368 ◽  
Author(s):  
J. Maza ◽  
P. G. Martin ◽  
J. R. P. Angel

1978 ◽  
Vol 83 ◽  
pp. 1021 ◽  
Author(s):  
B. Margon ◽  
T. W. Jones ◽  
J. F. C. Wardle

2002 ◽  
Vol 388 (2) ◽  
pp. 470-476 ◽  
Author(s):  
F. De Paolis ◽  
G. Ingrosso ◽  
A. A. Nucita

2014 ◽  
Vol 573 ◽  
pp. A69 ◽  
Author(s):  
Alicja Wierzcholska ◽  
Michał Ostrowski ◽  
Łukasz Stawarz ◽  
Stefan Wagner ◽  
Marcus Hauser

1998 ◽  
Vol 164 ◽  
pp. 165-166
Author(s):  
A. B. Pushkarev ◽  
D. C. Gabuzda

AbstractThe polarization electric vectors in the VLBI jets of BL Lacertae objects are typically aligned with the jet structure. If the jet radio emission is optically thin synchrotron emission, this implies that the magnetic field is perpendicular to the jet, usually interpreted as a signature of shocks. The distribution of polarization position angles in the VLBI core components appears to be bimodal, with the polarization angles either aligned with or perpendicular to the jet direction. In order to study the origin of this characteristic polarization structure, we have made VLBI polarization observations of all 34 sources in the Kühr and Schmidt sample of BL Lacertae objects.


2014 ◽  
Vol 570 ◽  
pp. A77 ◽  
Author(s):  
E. Pian ◽  
M. Türler ◽  
M. Fiocchi ◽  
R. Boissay ◽  
A. Bazzano ◽  
...  

2007 ◽  
Vol 475 (1) ◽  
pp. 199-207 ◽  
Author(s):  
K. Nilsson ◽  
M. Pasanen ◽  
L. O. Takalo ◽  
E. Lindfors ◽  
A. Berdyugin ◽  
...  

1998 ◽  
Vol 132 (1) ◽  
pp. 83-92 ◽  
Author(s):  
J. M. Bai ◽  
G. Z. Xie ◽  
K. H. Li ◽  
X. Zhang ◽  
W. W. Liu

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