Bolometric luminosities and brightness temperatures of BL Lac Objects and FR I radio galaxies

2012 ◽  
Vol 50 (1) ◽  
pp. 96-100 ◽  
Author(s):  
P. Seal Braun
1996 ◽  
Vol 175 ◽  
pp. 47-48
Author(s):  
A. Sillanpää ◽  
L. Takalo ◽  
K. Nilsson ◽  
T. Pursimo ◽  
P. Teerikorpi ◽  
...  

A widely accepted model for BL Lac objects is that they are radio galaxies with a relativistic jet pointing almost directly towards us. But we need a clear trigger mechanism for these jets. One possibility is the close interaction between the BL Lac host and the closeby galaxies (e.g. Heckman et al. 1986). This interaction has been seen many times in the case of quasars (Hutchings et al. 1989) but not so much is known about the close surroundings of the BL Lac objects although there has been some pioneer work like Stickel et al. (1993). The problem has usually been that the images are not deep enough and that the seeing has not been so good. To clarify the situation we have started an observing program to get very deep images in the sub-arcsecond seeing conditions from the whole 1 Jy sample (Stickel et al. 1991) of BL Lac objects. The aims of this study are: 1. to search for very close companions to the BL Lacs, 2. to study the large scale galaxy clustering around the BL Lacs and 3. to study the BL Lac hosts themselves.


1998 ◽  
Vol 164 ◽  
pp. 171-172
Author(s):  
M. Bondi ◽  
D. Dallacasa ◽  
M. J. M. Marchã ◽  
C. Stanghellini

AbstractWe present first results from a new sample of low radio luminosity flat spectrum radio galaxies.


1983 ◽  
Vol 5 (1) ◽  
pp. 2-83 ◽  
Author(s):  
Belinda J. Wilkes ◽  
Alan E. Wright ◽  
David L. Jauncey ◽  
Bruce A. Peterson

We present here the low-dispersion optical spectra of 295 QSO candidates. The great majority of the objects were originally selected as QSOs from the Parkes 2700 MHz radio survey, although we have also included spectra of several optically selected QSOs. A few of the QSO candidates are now better described as radio galaxies and BL Lac objects. This collection of spectra is not suitable for statistical studies unless due consideration is given to selection effects.


2001 ◽  
Vol 182 ◽  
pp. 105-111
Author(s):  
Stefan J. Wagner

AbstractIntraday variability is detected in Blazars throughout the electromagnetic spectrum. Only radio emission is affected by interstellar scintillation. The characteristics of variability observed at different frequencies are often similar and suggest that intrinsic variations also contribute to the changes detected in the radio wavelength regime. This in turn implies very high brightness temperatures.Unambiguous signatures of scintillation and of intrinsic changes have been identified. The properties of intrinsic variations are reviewed to illustrate their potential contribution to variability in the radio domain. Such intrinsic changes need to be discriminated against when studying scintillation in quasars and BL Lac objects. Observations of scintillating sources and of sources with significant intrinsic IDV suggest interesting modifications to the standard paradigm of AGN.


1983 ◽  
Vol 6 ◽  
pp. 443-457
Author(s):  
M.S. Longair

I have been invited to present a brief review of optical, infrared and ultraviolet observations of active nuclei. I will only describe a small sub-set of these observations, in particular those which I believe are most likely to be important in elucidating the properties of the central energy source to which we attribute the origin of all high energy phenomena. I will therefore restrict my remarks to certain aspects of BL Lac objects, optically violently variable quasars, quasars, Seyfert I galaxies and broad line radio galaxies. If we could understand these systems, we should be able to account for most other types of active nuclei, the Seyfert II galaxies, narrow line radio galaxies, all other types of Markarian galaxy, compact blue galaxy, etc. In my view, the recent observations of NGC 4151 provide us with a benchmark against which we should measure all other observations of active nuclei.


2008 ◽  
Vol 120 (867) ◽  
pp. 477-486 ◽  
Author(s):  
Z. H. Xie ◽  
J. M. Hao ◽  
L. M. Du ◽  
X. Zhang ◽  
Z. L. Jia
Keyword(s):  

2015 ◽  
Vol 357 (2) ◽  
Author(s):  
Yongyun Chen ◽  
Xiong Zhang ◽  
Haojing Zhang ◽  
Dingrong Xiong ◽  
Xiaoling Yu ◽  
...  
Keyword(s):  

1996 ◽  
Vol 175 ◽  
pp. 323-324
Author(s):  
J.E. Pesce ◽  
R. Falomo ◽  
G. Fasano ◽  
R. Scarpa

In the unified schemes of AGNs BL Lac objects are believed to be Fanaroff-Riley (FR) type I radio galaxies with a relativistic jet aligned to the observer's line of sight (e.g. Urry & Padovani 1995). Kollgaard et al. (1992) and Owen et al. (1995) suggest some FR II sources can also be BL Lac parents. Clearly, isotropic properties such as the galaxy environment of both beamed and unbeamed objects should be identical.


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