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相关论文: BL Lac evolution revisited

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The most elusive and extreme sub-class of active galactic nuclei (AGNs), known as BL Lac objects, shows features that can only be explained as the result of relativistic effects occurring in jets pointing at a small angle with respect to…

星系天体物理 · 物理学 2020-09-09 F. Massaro , A. Capetti , A. Paggi , R. D. Baldi , A. Tramacere , I. Pillitteri , R. Campana

BL Lac objects are active nuclei, hosted in massive elliptical galaxies, the emission of which is dominated by a relativistic jet closely aligned with the line of sight. This implies the existence of a parent population of sources with a…

高能天体物理现象 · 物理学 2016-11-26 Renato Falomo , Elena Pian , Aldo Treves

The unification of X-ray and radio selected BL Lacs has been an outstanding problem in the blazar research in the past years. Recent investigations have shown that the gap between the two classes can be filled with intermediate objects and…

天体物理学 · 物理学 2011-05-23 V. Beckmann , D. Engels , N. Bade , O. Wucknitz

We explain the properties of X-ray selected BL Lacertae objects, under the assumption that they constitute the small minority of the BL Lac population with energy cutoff located in the UV/X-ray band, as suggested by their multifrequency…

天体物理学 · 物理学 2009-10-22 Paolo Padovani , Paolo Giommi

The past 20 years have seen phenomenal progress in our understanding of BL Lac objects. They form part of the blazar class, which are radio-loud AGN whose relativistic jets are aligned along our line of sight. Several critical milestones…

天体物理学 · 物理学 2007-05-23 C. Megan Urry

The concept of the evolutionary sequence of jetted active galactic nuclei (AGNs) has been challenged in the last few decades since AGN subclasses are considered to be different due to their viewing angle. In this paper, we collected a…

星系天体物理 · 物理学 2022-01-26 Evaristus U. Iyida , Christian I. Eze , Finbarr C. Odo

We present a new well defined sample of BL Lac objects selected from the ROSAT All-Sky Survey (RASS). The sample consists of 39 objects with 35 forming a flux limited sample down to f_X = 8 x 10^{-13} cgs, redshifts are known for 33 objects…

天体物理学 · 物理学 2007-05-23 N. Bade , V. Beckmann , N. G. Douglas , P. D. Barthel , D. Engels , L. Cordis , P. Nass , W. Voges

We investigate the luminosity evolution of the host galaxies of radio-loud AGN through Hubble Space Telescope imaging of 72 BL Lac objects, including new STIS imaging of nine z > 0.6 BL Lacs. With their intrinsically low accretion rates and…

天体物理学 · 物理学 2009-11-10 Matthew O'Dowd , C. Megan Urry

We review the main results from several radio, X-ray and multi-frequency surveys on the topic of cosmological evolution of BL Lacertae objects. Updated findings on BL Lac evolution following the recent identification of many sources in the…

天体物理学 · 物理学 2007-05-23 P. Giommi , A. Pellizzoni , M. Perri , P. Padovani

We have analysed optical spectra of BL Lacertae, the prototype of its class, to verify the presence and possible flux variations of its broad Ha line. We used the spectroscopic information also to investigate the question of its parent…

宇宙学与河外天体物理 · 物理学 2019-08-14 Alessandro Capetti , Claudia Raiteri , Sara Buttiglione

We present analysis of a new flux limited sample of 72 X-ray selected BL Lacertae objects with known redshifts for 59 of them. We find the more X-ray dominated BL Lac having negative evolution with redshift, while intermediate objects show…

天体物理学 · 物理学 2007-05-23 Volker Beckmann

The evolution of extragalactic radio sources has been a fundamental problem in the study of active galactic nuclei for many years. A standard evolutionary model has been created based on observations of a wide range of radio sources. In the…

星系天体物理 · 物理学 2017-12-04 Aleksandra Wołowska , Magdalena Kunert-Bajraszewska , Kunal Mooley , Gregg Hallinan

This article focuses on certain variability and emission characteristics of Active Galactic Nuclei (AGN), especially their radio-loud subset consisting of quasars, BL Lacs and $\gamma$-ray detected narrow-line Seyfert 1 galaxies, all of…

星系天体物理 · 物理学 2019-06-28 Gopal-Krishna , Silke Britzen , Paul Wiita

The cosmological evolution of X-ray-selected and optically selected Active Galactic Nuclei (AGNs) show different behaviours interpreted in terms of two different populations. The difference is evident mainly for low luminosity AGNs…

天体物理学 · 物理学 2009-11-13 D. Trevese , V. Zitelli , F. Vagnetti , K. Boutsia , G. M. Stirpe

This paper concerns the relationship of BLLacs and flat spectrum weak emission-line galaxies. We compare the weak emission-line galaxies and the BLLacs in a sample of 57 flat spectrum objects (Marcha et al. 1996), using high-frequency radio…

天体物理学 · 物理学 2007-05-23 J. Dennett-Thorpe , M. J. Marcha

Changing-look active galactic nuclei (AGNs) are a special class of AGNs that change their spectral type from type 1 to type 2 or vice versa. In recent years, a number of changing-look blazars (CLBs) were also reported, which transition…

高能天体物理现象 · 物理学 2024-03-04 Shi-Ju Kang , Bing Lyu , Qingwen Wu , Yong-Gang Zheng , Junhui Fan

Many properties of BL Lacs have become explicable in terms of the "relativistic beaming" hypothesis whereby BL Lacs are FR-1 radio galaxies viewed nearly along the jet axis. However, a possible problem with this model is that a transition…

天体物理学 · 物理学 2009-10-31 Travis A. Rector , John T. Stocke , Eric S. Perlman

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

Low Luminosity Active Galactic Nuclei (LLAGNs) are contaminated by the light of their host galaxies, thus they cannot be detected by the usual colour techniques. For this reason their evolution in cosmic time is poorly known. Variability is…

星系天体物理 · 物理学 2009-02-09 F. Vagnetti , K. Boutsia , D. Trevese

We present the results on the cosmological evolution of BL Lac objects as derived from a statistically complete sample of 44 BL Lacs selected from the X-ray bright tail of the REX survey. With this sample, we have investigated the…

天体物理学 · 物理学 2007-05-23 A. Caccianiga , T. Maccacaro , A. Wolter , R. Della Ceca , I. M. Gioia
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