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Related papers: On the minimum jet power of TEV BL Lac objects in …

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A hard TeV $\gamma$-ray component excess over the single-zone leptonic model prediction (TeV excess) is observed in the spectral energy distributions (SEDs) of some BL Lacs. Its origin is uncertain. We revisit this issue with four BL Lacs…

High Energy Astrophysical Phenomena · Physics 2022-02-09 Ji-Gui Cheng , Xiao-Li Huang , Ze-Rui Wang , Jian-Kun Huang , En-Wei Liang

In this paper we discuss models of the X-rays and TeV gamma-ray emission from BL Lac objects based on parallel electron-positron or electron-proton beams that form close to the central black hole owing to the strong electric fields…

Astrophysics · Physics 2011-02-11 Henric Krawczynski

BL Lac objects are the best candidates to study the jet properties since their spectral energy distributions (SEDs) are less contaminated by the emission from the accretion disk and external Compton processes. We compile the broadband SEDs…

High Energy Astrophysical Phenomena · Physics 2015-05-30 Jin Zhang , En-Wei Liang , Shuang-Nan Zhang , Jin-Ming Bai

The spectral energy distributions (SEDs) of certain BL Lac objects (BL Lacs) exhibit an additional hard $\gamma$-ray component in the TeV energy range that surpasses the predictions of the one-zone leptonic jet model. The origin of this…

High Energy Astrophysical Phenomena · Physics 2025-11-11 Ji-Shun Lian , Ze-Rui Wang , Jin Zhang

BL Lac objects are known to have very energetic jets pointing towards the observer under small viewing angles. Many of these show high luminosity over the whole energy range up to TeV, mostly classified as high-energy peaked BL Lac objects.…

High Energy Astrophysical Phenomena · Physics 2015-06-03 S. Kaufmann , S. J. Wagner , O. Tibolla

Broadband spectral energy distributions (SEDs) are complied from literature for 24 TeV BL Lac objects. Two SEDs, which are identified as low and high states with their flux densities at $1\ {\rm TeV}$ ($F_{1 TeV}$), are available for each…

High Energy Astrophysical Phenomena · Physics 2011-08-20 Jin Zhang , En-Wei Liang , Shuang-Nan Zhang , Jin-Ming Bai

Very high energy (VHE; $E \geq$ 100GeV) $\gamma-$ray from cosmological distances are attenuated by the extragalactic background light (EBL) in the IR to UV band. By contrasting measured versus intrinsic emission, the EBL photon density can…

High Energy Astrophysical Phenomena · Physics 2020-09-01 Longhua Qin , Jiancheng Wang , Quangui Gao , Weiwei Na , Huaizhen Li , Ju Ma , Jianping Yang

We fit the spectral energy distributions (SEDs) of a GeV-TeV FSRQ sample with the leptonic model. Their gamma_min of the relativistic electron distributions, which significantly affect the estimates of the jet properties, are constrained,…

High Energy Astrophysical Phenomena · Physics 2014-04-29 Jin Zhang , Xiao-Na Sun , En-Wei Liang , Rui-Jing Lu , Ye Lu , Shuang-Nan Zhang

TeV emission can be a common characteristic of low power blazars. This is in line with the sequence of blazars relating the observed bolometric luminosity with their overall spectral energy distribution. Detecting new TeV blazars, possibly…

Astrophysics · Physics 2009-11-10 G. Ghisellini

We investigate the physical properties of \textit{Fermi} TeV BL Lac objects jets by modeling the quasi-simultaneous spectral energy distribution of 29 \textit{Fermi} TeV BL Lacs in the frame of a one-zone leptonic synchrotron self-Compton…

High Energy Astrophysical Phenomena · Physics 2016-09-28 N. Ding , X. Zhang , D. R. Xiong , H. J. Zhang

The production site of gamma rays in blazars is closely related to their interaction with the photon fields surrounding the active galactic nucleus. In this paper, we discuss an indirect method that may help to unveil the presence of…

High Energy Astrophysical Phenomena · Physics 2022-02-21 L. Foffano , V. Vittorini , M. Tavani , E. Menegoni

Most modeling attempts of blazars use a small emission zone located close to the central black hole in order to explain the broad-band spectral energy distribution. Here we present a case where additionally to the small region a…

High Energy Astrophysical Phenomena · Physics 2017-08-09 Michael Zacharias , Stefan Wagner

Through the modelling of the Spectral Energy Distribution of blazars we can infer the physical parameters required to originate the flux we see. Then we can estimate the power of blazar jets in the form of matter and fields. These estimates…

Astrophysics · Physics 2009-06-23 G. Ghisellini

We study the four BL Lac objects (RGB J0152+017, 1ES 0229+200, 1ES 0347-121 and PKS 0548-322) detected in the TeV band but not present in the 1FGL catalogue of the Fermi/Large Area Telescope. We analize the 24 months of LAT data deriving…

High Energy Astrophysical Phenomena · Physics 2015-05-19 F. Tavecchio , G. Ghisellini , G. Bonnoli , L. Foschini

The absorption of TeV $\gamma$-ray photons produced in relativistic jets by surrounding soft photon fields is a long-standing problem of jet physics. In some cases the most likely emission site close to the central black hole is ruled out…

High Energy Astrophysical Phenomena · Physics 2016-12-28 Michael Zacharias , Xuhui Chen , Stefan J. Wagner

Kinematical and luminosity relations for black-hole jet sources are reviewed. If the TeV flares observed from PKS 2155-304 in 2006 July are assumed to originate from a black hole with mass $\approx 10^8 M_8 M_\odot$, then the $\sim 5$…

Astrophysics · Physics 2008-10-08 Charles D. Dermer , Justin D. Finke , Govind Menon

The TeV emission of low power BL Lac objects has been established by the detection of an handful of them. The knowledge of the level of the TeV emission and its spectrum can shed light on the particle acceleration mechanisms, and it is…

Astrophysics · Physics 2009-11-07 L. Costamante , G. Ghisellini

We present the first search for pair production of isolated jets of charged leptons in association with a large imbalance in transverse energy in ppbar collisions using 5.8 fb^-1 of integrated luminosity collected by the D0 detector at the…

High Energy Physics - Experiment · Physics 2010-12-03 D0 Collaboration , V. Abazov et al.

We estimate the masses of massive black holes in BL Lac objects from their host galaxy luminosity. The power of jets and central optical ionizing luminosity for a sample of BL Lac objects are derived from their extended radio emission and…

Astrophysics · Physics 2009-11-10 Xinwu Cao

The Galactic high-mass X-ray binary and jet source (microquasar) LSI +61 303 has recently been detected at TeV gamma-ray energies by the MAGIC telescope. We have applied a time-dependent leptonic jet model to the broadband spectral energy…

Astrophysics · Physics 2011-02-11 Swati Gupta , Markus Boettcher
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