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Phase-Resolved Spectra of PSR B0525+21 and PSR B2020+28 | |
Chen, J. L.1,2![]() ![]() | |
2011-06-01 | |
Source Publication | JOURNAL OF ASTROPHYSICS AND ASTRONOMY
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Volume | 32Issue:1-2Pages:333-335 |
Contribution Rank | 1 |
Abstract | Using the published data of multi-frequency time-aligned pulse profiles from Kuzmin et al. (1998), we calculate the phase-resolved spectra of PSRs B0525+21 and B2020+28. The results reveal that conal-double pulsars have common 'M'-shaped phase-resolved spectra. |
Keyword | Pulsar Emission Mechanisms Phase-resolved Spectra |
Subtype | Article |
WOS Headings | Science & Technology ; Physical Sciences |
Indexed By | SCI |
Language | 英语 |
WOS Keyword | PULSAR EMISSION |
WOS Research Area | Astronomy & Astrophysics |
WOS Subject | Astronomy & Astrophysics |
WOS ID | WOS:000294539300074 |
Citation statistics | |
Document Type | 期刊论文 |
Identifier | http://ir.xao.ac.cn/handle/45760611-7/838 |
Collection | 射电天文研究室_脉冲星研究团组 射电天文研究室 其它 |
Corresponding Author | Wang, H. G. |
Affiliation | 1.Xinjiang Astron Observ, Urumqi 830011, Xinjiang, Peoples R China 2.Chinese Acad Sci, Grad Univ, Beijing 100049, Peoples R China 3.Guangzhou Univ, Ctr Astrophys, Guangzhou 510006, Guangdong, Peoples R China |
First Author Affilication | Xinjiang Astronomical Observatory, Chinese Academy of Sciences |
Recommended Citation GB/T 7714 | Chen, J. L.,Wang, H. G.,Wang, N.. Phase-Resolved Spectra of PSR B0525+21 and PSR B2020+28[J]. JOURNAL OF ASTROPHYSICS AND ASTRONOMY,2011,32(1-2):333-335. |
APA | Chen, J. L.,Wang, H. G.,&Wang, N..(2011).Phase-Resolved Spectra of PSR B0525+21 and PSR B2020+28.JOURNAL OF ASTROPHYSICS AND ASTRONOMY,32(1-2),333-335. |
MLA | Chen, J. L.,et al."Phase-Resolved Spectra of PSR B0525+21 and PSR B2020+28".JOURNAL OF ASTROPHYSICS AND ASTRONOMY 32.1-2(2011):333-335. |
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Chen-2011-Phase-Reso(115KB) | 期刊论文 | 出版稿 | 开放获取 | CC BY-NC-SA | View Application Full Text |
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