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相关论文: Spectral energy distributions and high-energy emis…

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We found significant correlations between the arrival directions of the highest energy photons (E>10 GeV) observed by EGRET and positions of the BL Lac type objects (BL Lacs). The observed correlations imply that not less than three per…

天体物理学 · 物理学 2008-11-26 D. S. Gorbunov , P. G. Tinyakov , I. I. Tkachev , S. V. Troitsky

We present BeppoSAX LECS, MECS, and PDS spectra of eleven X-ray selected BL Lacertae objects. Combining these sources with the ones presented elsewhere we have a sample of 21 BL Lacs from the Einstein Medium Sensitivity and Einstein Slew…

天体物理学 · 物理学 2009-11-07 V. Beckmann , A. Wolter , A. Celotti , L. Costamante , G. Ghisellini , T. Maccacaro , G. Tagliaferri

In current theoretical models of the blazar subclass of active galaxies, the broadband emission consists of two components: a low-frequency synchrotron component with a peak in the IR to X-ray band, and a high-frequency inverse Compton…

天体物理学 · 物理学 2009-10-31 Y. C. Lin

High-energy observations of extreme BL Lac objects, such as 1ES0229+200 or 1ES 0347-121, recently focused interest both for blazar and jet physics and for the implication on the extragalactic background light and intergalactic magnetic…

高能天体物理现象 · 物理学 2015-12-17 F. Tavecchio , G. Bonnoli

We calculate angular correlation function between ultra-high energy cosmic rays (UHECR) observed by Yakutsk and AGASA experiments, and most powerful BL Lacertae objects. We find significant correlations which correspond to the probability…

天体物理学 · 物理学 2009-11-06 P. G. Tinyakov , I. I. Tkachev

With their rapid, violent variability and broad featureless continuum emission, blazars have puzzled astronomers for over two decades. Today blazars represent the only extragalactic objects detected in high-energy gamma-rays. Their spectral…

天体物理学 · 物理学 2009-10-31 Eric S. Perlman

Extreme high-energy peaked BL Lac objects (EHBLs) are an emerging class of blazars with exceptional spectral properties. The non-thermal emission of the relativistic jet peaks in the spectral energy distribution (SED) plot with the…

高能天体物理现象 · 物理学 2019-07-19 L. Foffano , E. Prandini , A. Franceschini , S. Paiano

We consider various classes of persistent extragalactic astrophysical sources which have been suggested in literature as possible emitters of ultra-high-energy cosmic rays (UHECR). We compare the strength of the claimed correlations by a…

天体物理学 · 物理学 2008-11-26 D. S. Gorbunov , S. V. Troitsky

With the aim of testing recent claims for a particularly strong correlation between ultra-high energy cosmic rays (UHECRs), observed with the AGASA and the Yakutsk experiments, and a sample of BL Lacertae (BL Lacs), we here conduct a blind…

天体物理学 · 物理学 2009-11-10 Diego F. Torres , Stephen Reucroft , Olaf Reimer , Luis A. Anchordoqui

Blazars can be classified on the basis of their overall Spectral Energy Distribution (SED). BL Lac objects are usually divided in LBL or HBL (Low or High energy peaked BL Lacs), according to the peak frequency of the synchrotron emission,…

We present recent ROSAT, ASCA and SAX observations of intermediate BL Lac objects (IBLs), i.e. BL Lacs which are located between high-energy and low-energy peaked BL Lac objects with respect to alpha_rx. Both the statistical properties of…

天体物理学 · 物理学 2007-05-23 J. Siebert , W. Brinkmann , S. A. Laurent-Muehleisen

Most of the extragalactic sources detected at TeV energies are BL Lac objects. They belong to the subclass of "high frequency peaked BL Lacs" (HBLs) exhibiting spectral energy distributions with a lower energy peak in the X-ray band; this…

高能天体物理现象 · 物理学 2015-06-04 F. Massaro , A. Paggi , M. Elvis , A. Cavaliere

Extreme high-energy peaked BL Lac objects (EHBLs) are an emerging class of blazars with exceptional spectral properties. In blazars, the spectral energy distribution (SED) is dominated by the non-thermal emission of the relativistic jet,…

高能天体物理现象 · 物理学 2019-07-31 L. Foffano , E. Prandini , A. Franceschini , S. Paiano

We analyze the existing evidence that BL Lacertae objects (BL Lacs) are sources of the highest-energy cosmic rays. We argue that three independent signatures observed in the real data -- (1) improvement of correlations with corrections of…

高能物理 - 唯象学 · 物理学 2007-05-23 P. Tinyakov , I. Tkachev

The majority of the extragalactic sources yet detected at TeV photon energies belong to the class of "high frequency peaked BL Lacs" (HBLs) that exhibit a spectral energy distribution with a lower peak in the X-ray band. Such spectra are…

高能天体物理现象 · 物理学 2015-06-04 F. Massaro , A. Paggi , A. Cavaliere

High energy observations of extreme BL Lac objects, such as 1ES 0229+200 or 1ES 0347-121, recently focused interest both for blazar and jet physics and for the implication on the extragalactic background light and intergalactic magnetic…

高能天体物理现象 · 物理学 2015-06-25 Giacomo Bonnoli , Fabrizio Tavecchio , Gabriele Ghisellini , Tullia Sbarrato

Average Spectral Energy Distributions (SED) for different subgroups of blazars are derived from available homogeneous (but small) data sets, including the gamma-ray band. Comparing Flat Spectrum Radio Quasars (FSRQ) with BL Lacs extracted…

天体物理学 · 物理学 2007-05-23 Laura Maraschi , Giovanni Fossati

The extragalactic $\gamma$-ray sky is dominated by blazars and their study plays an important role in understanding jet physics, cosmic evolution history and origin of ultra high energy cosmic rays. In this work, we study a large sample of…

高能天体物理现象 · 物理学 2022-05-23 Muhammad Shahzad Anjum , Liang Chen , Minfeng Gu

We selected a sample of 437 BL Lac objects, taken from the RomaBZCat catalogue, for which spectroscopic information and SDSS photometry is available. We propose a new classification of BL Lacs in which the sources' type is not defined only…

高能天体物理现象 · 物理学 2015-06-04 Enrico Massaro , Roberto Nesci , Silvia Piranomonte

We study the X-ray spectra of 85 BL Lacertae objects using the hardness ratios as given in the WGA catalogue of {\it ROSAT} sources. This sample includes all WGA BL Lacs with high-quality data and comprises about 50 per cent of presently…

天体物理学 · 物理学 2015-06-24 Paolo Padovani , Paolo Giommi
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