耀变体的射线特性

IF 0.7 4区物理与天体物理 Q4 ASTRONOMY & ASTROPHYSICS

Astrophysics Pub Date : 2025-04-23 DOI:10.1007/s10511-025-09854-5

G. M. Paronyan

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引用次数: 0

摘要

对来自BZCAT星表的耀变体样本的分析表明，这些天体表现出一些特殊的特性，如强射电发射、光学和射电变异性、连续光谱、偏振和高亮度等。最初，该目录包括具有光学变异性和强射电发射的天体，特别是BL Lacertae （BLL）天体和平谱射电类星体（FSRQ）)。除了上述性质外，48%的耀变体还会发出x射线。本研究调查了通过我们的分析和计算确定的耀变体的x射线特性和其他特征。

本文章由计算机程序翻译，如有差异，请以英文原文为准。

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Ray Properties of Blazars

An analysis of the blazar sample from the BZCAT catalog reveals that these objects exhibit such special properties, as strong radio emission, optical and radio variability, continuous optical spectra, polarization, and high luminosity, among others. Initially, the catalog included objects with optical variability and strong radio emission, specifically BL Lacertae (BLL) objects and flat-spectrum radio quasars (FSRQ)). Along with the above properties, 48% of blazars produce X-ray emission. This study investigates the X-ray properties and other characteristics of blazars determined through our analyses and calculations.

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来源期刊

Astrophysics 地学天文-天文与天体物理

CiteScore

0.90

自引率

20.00%

发文量

审稿时长

6-12 weeks

期刊介绍： Astrophysics (Ap) is a peer-reviewed scientific journal which publishes research in theoretical and observational astrophysics. Founded by V.A.Ambartsumian in 1965 Astrophysics is one of the international astronomy journals. The journal covers space astrophysics, stellar and galactic evolution, solar physics, stellar and planetary atmospheres, interstellar matter. Additional subjects include chemical composition and internal structure of stars, quasars and pulsars, developments in modern cosmology and radiative transfer.