低音。会讲。尺度≤100 - 200pc的AGNs核毫米波连续发射特性目录

IF 8.6 1区 物理与天体物理 Q1 ASTRONOMY & ASTROPHYSICS Astrophysical Journal Supplement Series Pub Date : 2023-11-01 DOI:10.3847/1538-4365/acf467
Taiki Kawamuro, Claudio Ricci, Richard F. Mushotzky, Masatoshi Imanishi, Franz E. Bauer, Federica Ricci, Michael J. Koss, George C. Privon, Benny Trakhtenbrot, Takuma Izumi, Kohei Ichikawa, Alejandra F. Rojas, Krista Lynne Smith, Taro Shimizu, Kyuseok Oh, Jakob S. den Brok, Shunsuke Baba, Mislav Baloković, Chin-Shin Chang, Darshan Kakkad, Ryan W. Pfeifle, Matthew J. Temple, Yoshihiro Ueda, Fiona Harrison, Meredith C. Powell, Daniel Stern, Meg Urry, David B. Sanders
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引用次数: 0

摘要

摘要本文给出了98附近(z <从70个月的Swift/BAT硬x射线目录中选择的活动星系核(agn),精确地确定了x射线光谱特性和亚弧秒分辨率的阿塔卡马大毫米/亚毫米阵列波段6 (211-275 GHz)观测到2021年4月。由于硬x射线(>10 keV)的选择,该样品对于至少达到康普顿厚级遮挡的遮挡系统几乎是无偏的,并且提供了最多数量的具有高物理分辨率毫米波数据(> 100 - 200pc)的agn。我们的星表报告了在1.3 mm (230 GHz)处的发射峰坐标、光谱指数、峰值通量和光度。此外,还提供高分辨率毫米波图像。利用这些图像并创建毫米波发射的径向表面亮度曲线,我们识别了从中心源延伸的发射和孤立的斑点状发射。指示这些发射特征存在的标志被制成表格。在90个显著检测到核发射的agn中,37个agn(≈41%)似乎同时具有扩展或斑点状成分或其中一种成分。我们特别研究了具有良好分辨率的毫米波成分的AGN,发现它们似乎有各种各样的起源(即射流、射电瓣、次级AGN、星团、窄线区域、星系盘、活跃的恒星形成区或AGN驱动的外流),并且一些成分的起源目前尚不清楚。
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BASS. XXXIV. A Catalog of the Nuclear Millimeter-wave Continuum Emission Properties of AGNs Constrained on Scales ≤ 100–200 pc
Abstract We present a catalog of the millimeter-wave (mm-wave) continuum properties of 98 nearby ( z < 0.05) active galactic nuclei (AGNs) selected from the 70 month Swift/BAT hard-X-ray catalog that have precisely determined X-ray spectral properties and subarcsecond-resolution Atacama Large Millimeter/submillimeter Array Band 6 (211–275 GHz) observations as of 2021 April. Due to the hard-X-ray (>10 keV) selection, the sample is nearly unbiased for obscured systems at least up to Compton-thick-level obscuration, and provides the largest number of AGNs with high-physical-resolution mm-wave data (≲100–200 pc). Our catalog reports emission peak coordinates, spectral indices, and peak fluxes and luminosities at 1.3 mm (230 GHz). Additionally, high-resolution mm-wave images are provided. Using the images and creating radial surface brightness profiles of mm-wave emission, we identify emission extending from the central sources and isolated blob-like emission. Flags indicating the presence of these emission features are tabulated. Among 90 AGNs with significant detections of nuclear emission, 37 AGNs (≈41%) appear to have both or one of extended or blob-like components. We, in particular, investigate AGNs that show well-resolved mm-wave components and find that these seem to have a variety of origins (i.e., a jet, radio lobes, a secondary AGN, stellar clusters, a narrow-line region, galaxy disk, active star formation regions, or AGN-driven outflows), and some components have currently unclear origins.
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来源期刊
Astrophysical Journal Supplement Series
Astrophysical Journal Supplement Series 地学天文-天文与天体物理
CiteScore
14.50
自引率
5.70%
发文量
264
审稿时长
2 months
期刊介绍: The Astrophysical Journal Supplement (ApJS) serves as an open-access journal that publishes significant articles featuring extensive data or calculations in the field of astrophysics. It also facilitates Special Issues, presenting thematically related papers simultaneously in a single volume.
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