Studies of Active Galaxies in Byurakan: Recent Results

A. Mickaelian, H. Abrahamyan, G. Paronyan, G. Mikayelyan, M. Gyulzadyan
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引用次数: 4

Abstract

We present the recent results of studies on active galaxies (both AGN and Starbursts) by the Extragalactic group of Byurakan Astrophysical Observatory (BAO) Research Department “Astronomical Surveys”. The research has been carried out in 2017-2019 and the results are published in 2018-2019. These studies are characterized by multiwavelength approach to statistical analysis of large amount of data obtained in different wavelengths; from X-ray to radio. Results on HRC/BHRC sample objects (optical identifications of ROSAT X-ray sources), studies of Markarian galaxies in UV and multiwavelength SEDs, abundance and star formation determinations in Mrk galaxies from SDSS spectra, revised optical classification of “LINERs”, study and classification of SDSS spectra for Byurakan-IRAS Galaxies, summary of observations and study of Byurakan-IRAS Galaxies (BIG objects), discovery of new bright ULIRGs from the IRAS PSC/FSC Combined Catalogue and their spectral classification, radio variable sources at 1400 MHz and their optical variability, classification of BZCAT objects having uncertain types (BZU objects), and optical variability of blazars are presented.
比拉坎活跃星系的研究:最新成果
本文介绍了比尤拉坎天体物理天文台(BAO)研究部星系外小组对活动星系(AGN和星暴)的最新研究结果。该研究于2017-2019年进行,结果于2018-2019年发表。这些研究的特点是采用多波长方法对在不同波长获得的大量数据进行统计分析;从x射线到无线电。HRC/BHRC样品天体的结果(ROSAT x射线源的光学识别)、紫外和多波长SEDs中Markarian星系的研究、SDSS光谱中Mrk星系丰度和恒星形成的确定、“liner”的修正光学分类、Byurakan-IRAS星系SDSS光谱的研究和分类、Byurakan-IRAS星系(BIG天体)的观测和研究总结、本文介绍了在IRAS PSC/FSC联合星表中新发现的明亮ulrgs及其光谱分类、1400 MHz射电变源及其光学变异性、类型不确定的BZCAT天体(BZU天体)的分类以及blazar的光学变异性。
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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