Estimation of absolute magnitude-dependent Galactic model parameters in intermediate latitude with SDSS and SCUSS
文献类型：期刊论文
| 作者 | Jia, Yunpeng1; Du, Cuihua1; Wu, Zhenyu2; Peng, Xiyan2; Ma, Jun2; Zhou, Xu2; Fan, Xiaohui3,4; Fan, Zhou2; Jing, Yipeng5; Jiang, Zhaoji2 |
| 刊名 | MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
 |
| 出版日期 | 2014-06-01 |
| 卷号 | 441期号:1页码:503-512 |
| 关键词 | Galaxy: disc Galaxy: fundamental parameters Galaxy: halo Galaxy: structure |
| 通讯作者 | 沈世银 |
| 英文摘要 | Based on the Sloan Digital Sky Survey and South Galactic Cap of u-band Sky Survey (SCUSS) early data, we use a star count method to estimate the Galactic structure parameters in an intermediate latitude with 10 180 main-sequence (MS) stars in an absolute magnitude interval of 4 <= M-r <= 13. We divide the absolute magnitude into five intervals, 4 <= M-r < 5, 5 <= M-r < 6, 6 <= M-r < 8, 8 <= M-r < 10 and 10 <= M-r <= 13, and estimate the Galactic structure parameters in each absolute magnitude interval to explore their possible variation with the absolute magnitude. Our study shows that the parameters depend on absolute magnitude. For the thin disc, the intrinsic faint MS stars have large local space density and they tend to stay close to the Galactic plane. A plausible explanation is that faint MS stars with long lifetime experience and long gravitational interaction time result in a short scaleheight. However, for the thick disc, the parameters show a complex trend with absolute magnitude, which may imply the complicated original of the thick disc. For the halo, the intrinsic faint MS stars have large local density and small axial ratio, which indicate a flattened inner halo and a more spherical outer halo. |
| WOS标题词 | Science & Technology ; Physical Sciences |
| 类目[WOS] | Astronomy & Astrophysics |
| 研究领域[WOS] | Astronomy & Astrophysics |
| 关键词[WOS] | DIGITAL SKY SURVEY ; STELLAR METALLICITY DISTRIBUTION ; PHOTOMETRIC SPACE DENSITIES ; TAIWAN-CONNECTICUT SURVEY ; STAR COUNTS REDIVIVUS ; MILKY-WAY ; DATA RELEASE ; FAINT STARS ; THICK DISC ; LUMINOSITY FUNCTION |
| 收录类别 | SCI |
| 语种 | 英语 |
| WOS记录号 | WOS:000336249300035 |
| 公开日期 | 2015-02-14 |
| 源URL | [http://119.78.226.72//handle/331011/15798]  |
| 专题 | 上海天文台_星系宇宙学重点实验室 |
| 作者单位 | 1.Univ Chinese Acad Sci, Sch Phys, Beijing 100049, Peoples R China 2.Chinese Acad Sci, Key Lab Opt Astron, Natl Astron Observ, Beijing 100012, Peoples R China 3.Univ Arizona, Dept Astron, Tucson, AZ 85721 USA 4.Univ Arizona, Steward Observ, Tucson, AZ 85721 USA 5.Shanghai Jiao Tong Univ, Dept Phys & Astron, Shanghai 200240, Peoples R China 6.Chinese Acad Sci, Shanghai Astron Observ, Shanghai 200030, Peoples R China |
| 推荐引用方式 GB/T 7714 | Jia, Yunpeng,Du, Cuihua,Wu, Zhenyu,et al. Estimation of absolute magnitude-dependent Galactic model parameters in intermediate latitude with SDSS and SCUSS[J]. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY,2014,441(1):503-512. |
| APA | Jia, Yunpeng.,Du, Cuihua.,Wu, Zhenyu.,Peng, Xiyan.,Ma, Jun.,...&Zhou, Zhimin.(2014).Estimation of absolute magnitude-dependent Galactic model parameters in intermediate latitude with SDSS and SCUSS.MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY,441(1),503-512. |
| MLA | Jia, Yunpeng,et al."Estimation of absolute magnitude-dependent Galactic model parameters in intermediate latitude with SDSS and SCUSS".MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY 441.1(2014):503-512. |
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