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Multi-frequency observations of PSR B 0329+54
ESAMUDIN Ali1,2; WU Xin-ji3,4; ZHANG Jin1,2; WANG Na1,2,3,4; KANG Lian-sheng5; JIN Sheng-zheng2,5; ZHANG Hong-bo1,2; WANG Wei-xia1,2
2000-10
Source PublicationChinese Astronomy and Astrophysics
ISSN0275-1062
Volume24Issue:4Pages:467-472
Contribution Rank1
AbstractWe present the results of observations of the pulsar PSR B0329+54 at 0.327, 1.5, 2.3, 4.8 and 8.4 GHz during 1999 between 03-12 and 06-08, using the 25-m radio telescope of NAOC Urumqi Station. The spectrum shows a bend, the spectral index is 1.59 at the low frequency end, and 2.45 at the high frequency end. The angular width of the average pulse profile and the angular separation between two weak peaks both decrease with increasing frequency.
KeywordPulsar Radio Spectrum Multi-frequency Observation
Subject Area致密天体、高能和基础物理
DOI10.1016/S0275-1062(00)00077-1
URL查看原文
Indexed BySCI
Language英语
Funding Project脉冲星研究团组
WOS IDWOS:000165799700008
Funding OrganizationNational Natural Science Foundation
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Document Type期刊论文
Identifierhttp://ir.xao.ac.cn/handle/45760611-7/84
Collection射电天文研究室_脉冲星研究团组
科研仪器设备产出_利用南山26米射电望远镜(NSRT)观测数据的文章
Affiliation1.Urumqi Astronomical Station, Urumqi, 830011
2.National Astronomical Observaton’es, Chinese Academy of Sciences, Beijing 100012
3.Department of Geophysics, Peking University, Beijing 100871
4.CAS-Peking University Joint Beijing Astrophysical Center, Beijing 100871
5.Beijing Astronomical Observatory, Chinese Academy of Sciences, Beijing 100012
First Author AffilicationXinjiang Astronomical Observatory, Chinese Academy of Sciences
Recommended Citation
GB/T 7714
ESAMUDIN Ali,WU Xin-ji,ZHANG Jin,et al. Multi-frequency observations of PSR B 0329+54[J]. Chinese Astronomy and Astrophysics,2000,24(4):467-472.
APA ESAMUDIN Ali.,WU Xin-ji.,ZHANG Jin.,WANG Na.,KANG Lian-sheng.,...&WANG Wei-xia.(2000).Multi-frequency observations of PSR B 0329+54.Chinese Astronomy and Astrophysics,24(4),467-472.
MLA ESAMUDIN Ali,et al."Multi-frequency observations of PSR B 0329+54".Chinese Astronomy and Astrophysics 24.4(2000):467-472.
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