New CCD photometry of asteroid (1028) Lydina
文献类型:期刊论文
| 作者 | Wang YB(王夷博); Wang XB(王晓彬); Wang XB(王晓彬) ; Wang YB(王夷博)
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| 刊名 | RESEARCH IN ASTRONOMY AND ASTROPHYSICS
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| 出版日期 | 2012-12 |
| 卷号 | 12期号:12页码:1714-1722 |
| 关键词 | asteroids: photometric observation: rotation period pole orientation: tri-axial ellipsoid |
| ISSN号 | 1674-4527 |
| 产权排序 | 第一完成单位 |
| 通讯作者 | Wang, YB (reprint author), Chinese Acad Sci, Yunnan Observ, Natl Astron Observ, Kunming 650011, Peoples R China. |
| 英文摘要 | New CCD photometric observations for asteroid (1028) Lydina, carried out with the 1-m and 2.4-m telescopes at Yunnan Observatory from 2011 December 19 to 2012 February 3, are presented. Using the new light curves, the rotation period of 11.680 +/- 0.001 hours is derived with the Phase Dispersion Minimization (PDM) method. In addition, using the Amplitude-Aspect method, the elementary results of the pole orientation of asteroid (1028) Lydina are obtained: lambda(p) = 111 degrees(+4 degrees)(-4 degrees), beta(p)=31 degrees(+4 degrees)(-5 degrees). Meanwhile, the axial ratios of the tri-axial ellipsoid are estimated: a/b = 1.77(-0:08)(+0.10) and b/c = 1.17(-0.09)(+0.07). |
| 学科主题 | Astronomy & Astrophysics |
| 类目[WOS] | Astronomy & Astrophysics |
| 研究领域[WOS] | Astronomy & Astrophysics |
| 关键词[WOS] | POLE DETERMINATION ; ROTATION |
| 收录类别 | SCI |
| 原文出处 | http://iopscience.iop.org/1674-4527/12/12/013/ |
| 语种 | 英语 |
| WOS记录号 | WOS:000313011000013 |
| 公开日期 | 2016-05-03 |
| 源URL | [http://ir.ynao.ac.cn/handle/114a53/6789] ![]() |
| 专题 | 云南天文台_系外行星研究组 云南天文台_中国科学院天体结构与演化重点实验室 |
| 推荐引用方式 GB/T 7714 | Wang YB,Wang XB,Wang XB,et al. New CCD photometry of asteroid (1028) Lydina[J]. RESEARCH IN ASTRONOMY AND ASTROPHYSICS,2012,12(12):1714-1722. |
| APA | 王夷博,王晓彬,Wang XB,&Wang YB.(2012).New CCD photometry of asteroid (1028) Lydina.RESEARCH IN ASTRONOMY AND ASTROPHYSICS,12(12),1714-1722. |
| MLA | 王夷博,et al."New CCD photometry of asteroid (1028) Lydina".RESEARCH IN ASTRONOMY AND ASTROPHYSICS 12.12(2012):1714-1722. |
入库方式: OAI收割
来源:云南天文台
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