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Compact radio structure in the Seyfert nucleus of NGC 5929
Su BM(苏步美)1,3; Muxlow, TWB1; Pedlar, A1; Holloway, AJ2; Steffen, W2; Kukula, MJ4; Mutel, RL5; Su, BM(苏步美)
发表期刊MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
1996-04-15
卷号279期号:4页码:1111-1119
产权排序第3完成单位
收录类别SCI
关键词Galaxies Galaxies Galaxies Individual Nuclei Seyfert Radio Continuum Ngc 5329 Galaxies
摘要We present MERLIN and VLA radio measurements of the Seyfert galaxy NGC 5929 at 15, 8, 5, 1.6 and 0.4 GI-H. All measurements have subarcsecond angular resolution ranging from 0.6 arcsec at 0.4 GHz to 50 mas at 5 GHz, We confirm the triple structure reported in earlier studies. The weak central source of the triplet is almost certainly associated with the active nucleus. It has a flat spectral index and is unresolved even at 50-mas resolution, consistent with a synchrotron-self-absorbed core. The two components which straddle the core have sizes of order 10 pc and have steep spectral indices, and hence can be considered as small radio 'lobes'. Both of these components show evidence for low-frequency turnovers at 0.4 GHz, which we interpret as evidence for free-free absorption by ionized gas with an emission measure of similar to 10(5) pc cm(-6). As the north-eastern component shows greater free-free absorption than the south-western component, we propose that it is behind most of the narrow-line region (NLR) ionized gas, This implies that the nuclear collimated ejection is towards the observer in the south-west and away from the observer in the north-east.
语种英语
学科领域Astronomy & Astrophysics
文章类型Article
ISSN0035-8711
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WOS记录号WOS:A1996UG55300011
WOS研究方向Astronomy & Astrophysics
WOS类目Astronomy & Astrophysics
关键词[WOS]NARROW-LINE REGION ; GALAXY NGC-5929 ; EMISSION ; DRIVEN ; SCALE ; LOBES
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被引频次:24[WOS]   [WOS记录]     [WOS相关记录]
文献类型期刊论文
条目标识符http://ir.ynao.ac.cn/handle/114a53/4039
专题其他
通讯作者Su, BM(苏步美)
作者单位1.Nuffield Radio Astronomy Laboratories, University of Manchester, Jodrell Bank, Macclesfield, Cheshire SK11 9DL
2.Department of Physics & Astronomy, University of Manchester, Oxford Road, Manchester M13 9PL
3.Yunnan Observatory, Science Academy of China, PO Box 110, Kunming, China
4.School of Chemical & Physical Sicences, Liverpool John Moores University, Byrom Street, Liverpool L3 3AF
5.Department of Physics and Astronomy of Iowa University, USA
第一作者单位中国科学院云南天文台
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Su BM,Muxlow, TWB,Pedlar, A,et al. Compact radio structure in the Seyfert nucleus of NGC 5929[J]. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY,1996,279(4):1111-1119.
APA Su BM.,Muxlow, TWB.,Pedlar, A.,Holloway, AJ.,Steffen, W.,...&Su, BM.(1996).Compact radio structure in the Seyfert nucleus of NGC 5929.MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY,279(4),1111-1119.
MLA Su BM,et al."Compact radio structure in the Seyfert nucleus of NGC 5929".MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY 279.4(1996):1111-1119.
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