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相关论文: Unifying MeV-blazars with GeV-blazars

200 篇论文

Flat Spectrum Radio Quasars (FSRQs) are weak sources of very high energy (VHE; E>100 GeV) emission, despite exhibiting strong MeV-GeV emissions that dominate their radiative output. To date, only ten FSRQs have been detected at VHEs,…

高能天体物理现象 · 物理学 2025-04-15 Lekshmi Dathan , Pankaj Kushwaha

Flat spectrum radio quasars (FSRQs) constitute a class of jetted active galaxies characterized by a very luminous accretion disk, prominent and rapidly moving line-emitting cloud structures (Broad Line Region, BLR), and a surrounding dense…

高能天体物理现象 · 物理学 2025-09-16 MAGIC Collaboration

The flat spectrum radio quasars (FSRQs) are a sub-class of blazars characterised by prominent optical emission lines and a collimated large-scale jet along the observer line of sight. An X-ray spectral flattening has been reported in FSRQs…

高能天体物理现象 · 物理学 2021-06-16 Haritma Gaur , Prashanth Mohan , Ashwani Pandey

Flat Spectrum Radio Quasars (FSRQs) and BL Lac objects detected in the first three months of the Fermi survey neatly separate in the gamma-ray spectral index vs gamma-ray luminosity plane. BL Lac objects are less luminous and have harder…

宇宙学与河外天体物理 · 物理学 2015-05-13 G. Ghisellini , L. Maraschi , F. Tavecchio

The highest-energy blazars exhibit non-thermal radiation extending beyond 1 TeV with high luminosities and strong variabilities, indicating extreme particle acceleration in their relativistic jets. The gamma-ray spectra of blazars contain…

高能天体物理现象 · 物理学 2022-09-21 Qi Feng

Deviation of the gamma-ray energy spectra of Flat Spectrum Radio Quasars (FSRQs) from a simple power law has been previously observed but the cause of this remains unidentified. If the gamma-ray emission region is close to the central black…

高能天体物理现象 · 物理学 2015-06-11 Jonathan Harris , Michael K. Daniel , Paula M. Chadwick

The non-thermal spectra of blazars, observed from radio to GeV/TeV gamma-rays, reveal two pronounced components, both produced by radiation by energetic particles. One peaks in the IR - to soft X-ray band, radiating via the synchrotron…

天体物理学 · 物理学 2009-10-31 Tadayuki Takahashi , Greg Madejski , Hidetoshi Kubo

It is proposed that the spectra of so called 'MeV blazars' can be explained in terms of previously developed models of the external comptonization of accretion disk radiation provided that the structure of the inner and outer parts of the…

天体物理学 · 物理学 2020-11-25 W. Bednarek

In this paper we present a statistical analysis of the gamma-ray spectra of flat-spectrum radio quasars (FSRQ) compared to those of BL Lacs. The average spectra and possible systematic deviations from power-law behaviour are investigated by…

天体物理学 · 物理学 2009-10-30 M. Pohl , R. C. Hartman , B. B. Jones , P. Sreekumar

Flat Spectrum Radio Quasars (FSRQ) are the most powerful blazars in the gamma-ray band. Although they are supposed to be good candidates in producing high energy neutrinos, no secure detection of FSRQs has been obtained up to now, except…

高能天体物理现象 · 物理学 2020-10-14 C. Righi , A. Palladino , F. Tavecchio , F. Vissani

Blazar subclasses ranging from flat-spectrum radio quasars (FSRQs) through low-frequency-peaked BL Lac objects (LBLs) to high-frequency-peaked BL Lac objects (HBLs) exhibit a sequence of increasing spectral hardness with decreasing…

天体物理学 · 物理学 2009-11-06 M. Boettcher , C. D. Dermer

Blue quasars (BQs) are sources with strong broad emission lines and flat hard X-ray spectra, properties that resemble classical flat spectrum radio quasars (FSRQs), and high peak frequencies and steep soft X-ray spectra, properties that…

天体物理学 · 物理学 2009-10-31 Markos Georganopoulos

We study the dependence of nonthermal radiation spectra in OVV quasars on location of the low energy break in the electron/positron injection function. We show that the high energy spectra produced during the outbursts are presumably…

天体物理学 · 物理学 2007-05-23 M. Blazejowski , M. Sikora , R. Moderski , T. Bulik

The Fermi-LAT revealed that the census of the gamma-ray sky is dominated by blazars. Looking for a possible connection between radio and gamma-ray emission is a central issue for understanding the blazar physics, and various works were…

高能天体物理现象 · 物理学 2017-12-13 R. Lico , M. Giroletti , M. Orienti , L. Costamante , V. Pavlidou , F. D'Ammando , F. Tavecchio

We try to infer the location of the GeV emission region for 21 flat spectrum radio quasars (FSRQs) with quasi-simultaneous spectral energy distributions (SEDs), in which the SEDs of 21 FSRQs are reproduced by the one-zone leptonic model…

高能天体物理现象 · 物理学 2015-06-17 Gang Cao , Jiancheng Wang

We studied the rapid variability at GeV gamma rays of the flat-spectrum radio quasar PKS 1222+216, which was recently found by the MAGIC Cerenkov telescope to display very short variability (minutes time scale) at hundreds of GeV. We…

高能天体物理现象 · 物理学 2012-02-14 L. Foschini , G. Ghisellini , F. Tavecchio , G. Bonnoli , A. Stamerra

We have recently proposed a simplified scenario for blazars in which these sources are classified as flat-spectrum radio quasars or BL Lacs according to the prescriptions of unified schemes, and to a varying combination of Doppler boosted…

高能天体物理现象 · 物理学 2015-06-23 P. Padovani , P. Giommi

We propose and test a fairly simple idea that could account for the blazar sequence: all jets are launched with similar energy per baryon, independently of their power. For instance, flat-spectrum radio quasars (FSRQs), the most powerful…

高能天体物理现象 · 物理学 2021-01-13 Jesús M. Rueda-Becerril , Amanda O. Harrison , Dimitrios Giannios

We use the distributions of spectral indices of a large homogenous sample of Fermi-detected blazars to re-investigate the relationship between flat spectrum radio quasars (FSRQs) and subclasses of BL Lac objects (BL Lacs). We compute the…

高能天体物理现象 · 物理学 2020-07-20 E. U. Iyida , F. C. Odo , A. E. Chukwude , A. A. Ubachukwu

Based on a 10 years sample of gamma-ray flares of FSRQs collected with FERMI and AGILE, I report on this proceeding the advance on a statistical study of variability for a sample of more than 300 FSRQs. I will focus on waiting time between…

高能天体物理现象 · 物理学 2025-07-08 Luigi Pacciani