Transient Events in the Circumnuclear Regions of AGNs and Quasars As Sources of Imitations of Proper Motions

IF 1.1 4区 物理与天体物理 Q3 ASTRONOMY & ASTROPHYSICS
I. M. Khamitov, I. F. Bikmaev, M. R. Gilfanov, R. A. Sunyaev, P. S. Medvedev, M. A. Gorbachev
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Abstract

This paper is an extension of the study by Khamitov et al. (2022) with regard to the catalog and the astrophysical interpretation of the imitation of significant proper motions in active galactic nuclei (AGNs) and quasars based on data from the Gaia space observatory. We present a sample of SRG/eROSITA X-ray sources in the eastern Galactic hemisphere (\({0^{\circ}<l<180^{\circ}}\)) having significant proper motions in the Gaia EDR3 measurements with the confirmed extragalactic nature of the objects. The catalog consists of 248 extragalactic sources with spectroscopically measured redshifts. The catalog includes all of the objects available in the SIMBAD database and coincident with the identified optical counterpart within 0.5 arcsec. Eighteen sources with spectroscopically measured redshifts from observations with the Russian–Turkish 1.5-m telescope RTT-150 (Khamitov et al. 2022) have been additionally included in the catalog. The sources in the catalog are AGNs of various types (Sy1, Sy2, LINER), quasars, radio galaxies, and star-forming galaxies. The imitation of significant proper motions can be explained (by the VIM effect previously known in astrometry) by the presence of transient events on the line of sight in the vicinity of AGNs and quasars (within the Gaia optical resolution element). Among such astrophysical events are supernova outbursts, tidal disruption events in binary AGNs, the variability of high-mass supergiants, the presence of OB associations against the background of AGNs with a variable brightness, etc. The model of outbursts with a fast rise–exponential decay profile allows the variable positional parameters of most sources observed in Gaia to be described. This approach can be used as an independent way of detecting transient events in the vicinity of AGNs (on scales of several hundred parsecs in the plane of the sky) based on data from the SRG/eROSITA catalogs of X-ray sources and the optical Gaia catalog.

Abstract Image

作为固有运动限制源的agn和类星体环核区域瞬态事件
本文是Khamitov等人(2022)基于盖亚空间天文台数据对活动星系核(agn)和类星体中重要固有运动模拟的目录和天体物理学解释研究的延伸。我们在银河系东半球(\({0^{\circ}<l<180^{\circ}}\))提供了一个SRG/eROSITA x射线源样本,在盖亚EDR3测量中具有显著的固有运动,并证实了物体的河外性质。该目录包括248个星系外的源,光谱测量红移。该目录包括SIMBAD数据库中可用的所有对象,并且在0.5弧秒内与已识别的光学对应物一致。俄罗斯-土耳其1.5米望远镜RTT-150 (Khamitov et al. 2022)观测到的光谱测量红移的18个源已被额外列入目录。目录中的源是各种类型的agn (Sy1, Sy2, LINER),类星体,射电星系和恒星形成星系。重要的固有运动的模仿可以通过agn和类星体(在盖亚光学分辨率元件范围内)附近视线上的瞬态事件的存在来解释(通过天体测量中先前已知的VIM效应)。这些天体物理事件包括超新星爆发、双星agn中的潮汐破坏事件、高质量超巨星的可变性、在亮度可变的agn背景下OB关联的存在等。具有快速上升-指数衰减剖面的爆发模型允许描述在盖亚观测到的大多数源的可变位置参数。基于SRG/eROSITA x射线源目录和光学Gaia目录的数据,这种方法可以作为探测agn附近瞬变事件的一种独立方法(在天空平面上的数百秒差距范围内)。
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来源期刊
CiteScore
1.70
自引率
22.20%
发文量
0
审稿时长
6-12 weeks
期刊介绍: Astronomy Letters is an international peer reviewed journal that publishes the results of original research on all aspects of modern astronomy and astrophysics including high energy astrophysics, cosmology, space astronomy, theoretical astrophysics, radio astronomy, extragalactic astronomy, stellar astronomy, and investigation of the Solar system.
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