Discovery of a new supernova remnant G 150.3+4.5 | |
Gao, X. Y.![]() ![]() | |
刊名 | ASTRONOMY & ASTROPHYSICS
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2014-07-01 | |
卷号 | 567 |
关键词 | radio continuum: ISM ISM: supernova remnants |
英文摘要 | Context Large-scale radio continuum surveys have good potential for discovering new Galactic supernova remnants (SNRs). Surveys of the Galactic plane are often limited in the Galactic latitude of |b| similar to 5 degrees. SNRs at high latitudes, such as the Cygnus Loop or CIA 1. cannot be detected by surveys in such limited latitudes. Aims. Using the available Urumqi lambda 6 cm Galactic plane survey data, together with the maps from the extended ongoing lambda 6 cm medium latitude survey. WC Wish to discover new, SNRs in a large sky area. |
收录类别 | SCI |
语种 | 英语 |
WOS记录号 | WOS:000341185300149 |
内容类型 | 期刊论文 |
源URL | [http://ir.bao.ac.cn/handle/114a11/6562] ![]() |
专题 | 国家天文台_射电天文研究部 |
作者单位 | Chinese Acad Sci, Natl Astron Observ, Beijing 100012, Peoples R China |
推荐引用方式 GB/T 7714 | Gao, X. Y.,Han, J. L.. Discovery of a new supernova remnant G 150.3+4.5[J]. ASTRONOMY & ASTROPHYSICS,2014,567. |
APA | Gao, X. Y.,&Han, J. L..(2014).Discovery of a new supernova remnant G 150.3+4.5.ASTRONOMY & ASTROPHYSICS,567. |
MLA | Gao, X. Y.,et al."Discovery of a new supernova remnant G 150.3+4.5".ASTRONOMY & ASTROPHYSICS 567(2014). |
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