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Broad absorption line quasars (BAL QSOs) belong to a class of objects not well-understood as yet. Their UV spectra show BALs in the blue wings of the UV resonance lines, owing to ionized gas with outflow velocities up to 0.2 c. They can…

宇宙学与河外天体物理 · 物理学 2013-06-17 G. Bruni , D. Dallacasa , K. -H. Mack , F. M. Montenegro-Montes , J. I. González-Serrano , J. Holt , F. Jiménez-Luján

We investigate why BL Lacertae objects (BL Lacs) have values of the Ca H&K break (a stellar absorption feature) lower than low-power radio galaxies and if its use is justified to separate the two classes. For this purpose we relate this…

天体物理学 · 物理学 2009-11-07 H. Landt , P. Padovani , P. Giommi

With high-sensitivity kiloparsec-scale radio polarimetry, we can examine the jet-medium interactions and get a better understanding of the blazar divide in radio-loud (RL) AGN. We are analyzing the radio polarimetric observations with the…

星系天体物理 · 物理学 2023-04-25 Janhavi Baghel , P. Kharb , Silpa S. , Luis C. Ho , C. M. Harrison

If the transverse jet B fields observed in BL Lac objects on parsec scales represent the toroidal component of the jet B fields, this should give rise to rotation-measure gradients across the jets, due to the systematic change in the…

天体物理学 · 物理学 2007-05-23 D. C. Gabuzda , E. Murray , P. Cronin

We are using "broadband" (4.6 to 43 GHz) multi-frequency VLBA polarization observations of compact AGN to investigate the 3-D structure of their jet magnetic (B) fields. Observing at several frequencies, separated by short and long…

天体物理学 · 物理学 2008-02-01 Shane P. O'Sullivan , Denise C. Gabuzda

We interpret the linear polarization structures observed in extragalactic radio sources, even those oriented at oblique angles to the jet flows, to be due to oblique, relativistic shock fronts in the emitting regions. Many sources exhibit…

天体物理学 · 物理学 2007-05-23 H. D. Aller , M. F. Aller , P. A. Hughes

We investigate the pc-scale kinematics and kpc-scale radio morphology of the quasar PG 1302-102, which may harbour a sub-pc separation supermassive binary black hole system at its centre as inferred from optical variability. High-resolution…

高能天体物理现象 · 物理学 2015-11-23 E. Kun , S. Frey , K. É. Gabányi , S. Britzen , D. Cseh , L. Á. Gergely

The results of VLBI total intensity (I) and linear polarization (P) observations at 6cm are presented for ten radio bright BL Lacertae objects. These images complete first-epoch polarization observations for the 1-Jy sample of northern BL…

天体物理学 · 物理学 2009-11-10 D. C. Gabuzda , A. B. Pushkarev , T. V. Cawthorne

A new paradigm for active galactic jet kinematics has emerged through detailed investigations of BL Lac objects using very long baseline radio interferometry. In this new scheme, most, if not all, jet components appear to remain stationary…

宇宙学与河外天体物理 · 物理学 2012-06-20 Marios Karouzos , Silke Britzen , Arno Witzel , Anton J. Zensus , Andreas Eckart

We investigate the total flux density, spectral, polarization, and Faraday rotation variability of HST-1 in the M87 jet during the outburst from 2003 to 2007 through multi-epoch VLA observations at 8, 15, and 22 GHz. Contrary to the general…

宇宙学与河外天体物理 · 物理学 2015-05-28 Y. J. Chen , G. -Y. Zhao , Z. -Q. Shen

BL Lacertae is the prototype of the BL Lac class of active galactic nuclei, exhibiting intensive activity on parsec (pc) scales, such as intense core variability and multiple ejections of jet components. In particular, in previous works the…

高能天体物理现象 · 物理学 2015-06-11 Anderson Caproni , Zulema Abraham , Hektor Monteiro

In the framework of the unification scheme of radio-loud active galactic nuclei, BL Lac objects and quasars are the beamed end-on counterparts of low-power (FRI) and high-power (FRII) radio galaxies, respectively. Some BL Lacs have been…

星系天体物理 · 物理学 2015-06-18 Natalia Zywucka , Arti Goyal , Marek Jamrozy , Michal Ostrowski , Lukasz Stawarz

We report on multi-bands VLBA polarimetric observations of NRAO 530 in February 1997. Total intensity, EVPA distributions at all these frequencies are presented. Model fitting has been performed, from which the fitted southmost component A…

宇宙学与河外天体物理 · 物理学 2015-05-19 Y. J. Chen , Z. -Q. Shen , S. -W. Feng

We present first-epoch, milliarcsecond-scale linear polarization images at 15 GHz of 133 jets associated with AGN in the MOJAVE survey (Monitoring of Jets in Active Galactic Nuclei with VLBA Experiments). The sample consists of all known…

天体物理学 · 物理学 2009-09-29 M. L. Lister , D. C. Homan

We present a multi-frequency polarimetric study for the quasar 1604+159. The source was observed at the $L$ band with the American Very Long Baseline Array (VLBA) and the $L$, $X$, and $U$ bands with the Very Large Array (VLA). These…

星系天体物理 · 物理学 2024-08-14 Xu-Zhi Hu , Xiaoyu Hong , Wei Zhao , Liang Chen , Wei-Yang Wang , Linhui Wu

The Very Large Array has been used at five frequencies to study the structure and linear polarization of SS433 on scales as small as ~0.1" ~ 500 AU. Each jet consists of a sharp, curving ridge-line at the leading edge, plus significant…

天体物理学 · 物理学 2009-11-13 David H. Roberts , John F. C. Wardle , Scott L. Lipnick , Philip L. Selesnick , Simon Slutsky

We present new multi-epoch Very Long Baseline Array (VLBA) observations of a set of TeV blazars drawn from our VLBA program to monitor all TeV-detected high-frequency peaked BL Lac objects (HBLs) at parsec scales. Most of these sources are…

星系天体物理 · 物理学 2016-12-31 B. Glenn Piner , Philip G. Edwards

Hubble Space Telescope (HST) observations provide a novel way of testing unified models for FR I radio sources and BL Lac objects. The detection of extended dust discs in some radio galaxies provides information on their jet orientation.…

天体物理学 · 物理学 2009-10-31 Alessandro Capetti , Annalisa Celotti

We present the first polarimetric space VLBI imaging observations at 22 GHz. BL Lacertae was observed in 2013 November 10 with the RadioAstron space VLBI mission, including a ground array of 15 radio telescopes. The instrumental…

We collect multi-wavelength measurements of the nuclear emission of 20 low luminosity FR I radio-galaxies to test the viability of the FR I - BL Lac unifying model. Although poorly sampled, the Spectral Energy Distributions (SED) of FR Is…

天体物理学 · 物理学 2009-11-07 E. Trussoni , A. Capetti , A. Celotti , M. Chiaberge , L. Feretti