Compact Symmetric Objects. I. Toward a Comprehensive Bona Fide Catalog

被引:6
|
作者
Kiehlmann, S. [1 ,2 ]
Lister, M. L. [3 ]
Readhead, A. C. S. [4 ]
Liodakis, I. [5 ]
O'Neill, Sandra [4 ]
Pearson, T. J. [4 ]
Sheldahl, Evan [6 ]
Siemiginowska, Aneta [7 ]
Tassis, K. [1 ,2 ]
Taylor, G. B. [6 ]
Wilkinson, P. N. [8 ]
机构
[1] Fdn Res & Technol Hellas, Inst Astrophys, GR-70013 Iraklion, Greece
[2] Univ Crete, Inst Theoret & Computat Phys, Dept Phys, Iraklion 70013, Greece
[3] Purdue Univ, Dept Phys & Astron, 525 Northwestern Ave, W Lafayette, IN 47907 USA
[4] CALTECH, Owens Valley Radio Observ, Pasadena, CA 91125 USA
[5] Univ Turku, Finnish Ctr Astron ESO, Vesilinnantie 5, FI-20014 Turku, Finland
[6] Univ New Mexico, Dept Phys & Astron, Albuquerque, NM 87131 USA
[7] Ctr Astrophys Harvard & Smithsonian, 60 Garden St, Cambridge, MA 02138 USA
[8] Univ Manchester, Jodrell Bank Ctr Astrophys, Oxford Rd, Manchester M13 9PL, England
来源
ASTROPHYSICAL JOURNAL | 2024年 / 961卷 / 02期
基金
欧洲研究理事会; 美国国家航空航天局; 美国国家科学基金会;
关键词
SPECTRUM RADIO-SOURCES; ACTIVE GALACTIC NUCLEI; GAMMA-RAY EMISSION; MULTIFREQUENCY VLBI OBSERVATIONS; HIGH-ENERGY EMISSION; B3-VLA CSS SAMPLE; X-RAY; STEEP-SPECTRUM; DATA RELEASE; SKY SURVEY;
D O I
10.3847/1538-4357/ad0c56
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Compact symmetric objects (CSOs) are jetted active galactic nuclei (AGN) with overall projected size <1 kpc. The classification was introduced to distinguish these objects from the majority of compact jetted AGN in centimeter-wavelength very long baseline interferometry observations, where the observed emission is relativistically boosted toward the observer. The original classification criteria for CSOs were (i) evidence of emission on both sides of the center of activity and (ii) overall size <1 kpc. However, some relativistically boosted objects with jet axes close to the line of sight appear symmetric and have been misclassified as CSOs, thereby undermining the CSO classification. This is because two essential CSO properties, pointed out in the original papers, have been neglected: (iii) low variability and (iv) low apparent speeds along the jets. As a first step toward creating a comprehensive catalog of "bona fide" CSOs, we identify 79 bona fide CSOs, including 15 objects claimed as confirmed CSOs here for the first time, that match the CSO selection criteria. This sample of bona fide CSOs can be used for astrophysical studies of CSOs without contamination by misclassified CSOs. We show that the fraction of CSOs in complete flux density limited AGN samples with S-5GHz > 700 mJy is between (6.8 +/- 1.6)% and (8.5 +/- 1.8)%.
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页数:19
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