The distance and size of the red hypergiant NML Cygni from VLBA and VLA astrometry | |
Zhang, B.1,2![]() | |
刊名 | ASTRONOMY & ASTROPHYSICS
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2012-08-01 | |
卷号 | 544期号:1页码:1 |
关键词 | astrometry masers parallaxes proper motions stars: individual: NML Cyg supergiants |
英文摘要 | Context. The red hypergiant NML Cyg has been assumed to be at part of the Cyg OB2 association, although its distance has never been measured directly. A reliable distance is crucial to study the properties of this prominent star. For example, its luminosity, and hence its position on the H-R diagram, is critical information to determine its evolutionary status. In addition, a detection of the radio photosphere would be complementary to other methods of determining the stellar size. |
WOS标题词 | Science & Technology ; Physical Sciences |
类目[WOS] | Astronomy & Astrophysics |
研究领域[WOS] | Astronomy & Astrophysics |
关键词[WOS] | VY-CANIS-MAJORIS ; LATE-TYPE STARS ; PROPER MOTIONS ; DUST SHELLS ; TRIGONOMETRIC PARALLAXES ; CIRCUMSTELLAR ENVELOPE ; RADIO PHOTOSPHERES ; RADIATIVE-TRANSFER ; MASER EMISSION ; MILKY-WAY |
收录类别 | SCI |
语种 | 英语 |
WOS记录号 | WOS:000308290100042 |
内容类型 | 期刊论文 |
源URL | [http://119.78.226.72/handle/331011/18076] ![]() |
专题 | 上海天文台_VLBI研究室 |
作者单位 | 1.Max Planck Inst Radioastron, D-53121 Bonn, Germany 2.Chinese Acad Sci, Shanghai Astron Observ, Shanghai 200030, Peoples R China 3.Harvard Smithsonian Ctr Astrophys, Cambridge, MA 02138 USA 4.Nanjing Univ, Dept Astron, Nanjing 210093, Jiangsu, Peoples R China 5.Natl Radio Astron Observ, Socorro, NM 87801 USA |
推荐引用方式 GB/T 7714 | Zhang, B.,Reid, M. J.,Menten, K. M.,et al. The distance and size of the red hypergiant NML Cygni from VLBA and VLA astrometry[J]. ASTRONOMY & ASTROPHYSICS,2012,544(1):1. |
APA | Zhang, B.,Reid, M. J.,Menten, K. M.,Zheng, X. W.,&Brunthaler, A..(2012).The distance and size of the red hypergiant NML Cygni from VLBA and VLA astrometry.ASTRONOMY & ASTROPHYSICS,544(1),1. |
MLA | Zhang, B.,et al."The distance and size of the red hypergiant NML Cygni from VLBA and VLA astrometry".ASTRONOMY & ASTROPHYSICS 544.1(2012):1. |
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