CCD photometry of the BL Lacertae objects 1218+304, 1219+28, and 1727+50 - Point sources, associated nebulosity, and broad-band spectra

1981 ◽  
Vol 249 ◽  
pp. 3 ◽  
Author(s):  
D. Weistrop ◽  
R. F. Mushotzky ◽  
D. B. Shaffer ◽  
H. J. Reitsema ◽  
B. A. Smith
1996 ◽  
Vol 111 ◽  
pp. 1065 ◽  
Author(s):  
G. Z. Xie ◽  
Y. H. Zhang ◽  
K. H. Li ◽  
F. K. Liu ◽  
J. C. Wang ◽  
...  

2010 ◽  
Vol 327 (1) ◽  
pp. 35-58 ◽  
Author(s):  
L. Ma ◽  
G. Z. Xie ◽  
T. F. Yi ◽  
S. B. Zhou ◽  
K. H. Li ◽  
...  

1992 ◽  
Vol 80 ◽  
pp. 683 ◽  
Author(s):  
G. Z. Xie ◽  
K. H. Li ◽  
F. K. Liu ◽  
R. W. Lu ◽  
J. X. Wu ◽  
...  

2007 ◽  
Vol 133 (5) ◽  
pp. 1995-2000 ◽  
Author(s):  
X. Zhang ◽  
G. Zhao ◽  
Y. G. Zheng ◽  
L. Ma ◽  
Z. H. Xie ◽  
...  

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.


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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