KINEMATIC PROPERTIES OF DOUBLE-BARRED GALAXIES: SIMULATIONS VERSUS INTEGRAL-FIELD OBSERVATIONS
文献类型：期刊论文
| 作者 | Du,Min1; Debattista,Victor P.2; Shen,Juntai1; Cappellari,Michele3 |
| 刊名 | The Astrophysical Journal
 |
| 出版日期 | 2016-08-23 |
| 卷号 | 828期号:1 |
| 关键词 | galaxies: individual (NGC 2859, NGC 2950, NGC 3941, NGC 3384) galaxies: kinematics and dynamics galaxies: structure |
| ISSN号 | 0004-637X |
| DOI | 10.3847/0004-637X/828/1/14 |
| 英文摘要 | ABSTRACT Using high-resolution N-body simulations, we recently reported that a dynamically cool inner disk embedded in a hotter outer disk can naturally generate a steady double-barred (S2B) structure. Here we study the kinematics of these S2B simulations, and compare them to integral-field observations from ATLAS3D?and SAURON. We show that S2B galaxies exhibit several distinct kinematic features, namely: (1) significantly distorted isovelocity contours at the transition region between the two bars, (2) peaks in σLOS along the minor axis of inner bars, which we term “σ-humps,” that are often accompanied by ring/spiral-like features of increased σLOS, (3) anti-correlations in the region of the inner bar for certain orientations, and (4) rings of positive h4 when viewed at low inclinations. The most impressive of these features are the σ-humps; these evolve with the inner bar, oscillating in strength just as the inner bar does as it rotates relative to the outer bar. We show that, in cylindrical coordinates, the inner bar has similar streaming motions and velocity dispersion properties as normal large-scale bars, except for σz, which exhibits peaks on the minor axis, i.e., humps. These σz humps are responsible for producing the σ-humps. For three well-resolved early-type S2Bs (NGC 2859, NGC 2950, and NGC 3941) and a potential S2B candidate (NGC 3384), the S2B model qualitatively matches the integral-field data well, including the “σ-hollows” previously identified. We also discuss the kinematic effect of a nuclear disk in S2Bs. |
| 语种 | 英语 |
| WOS记录号 | IOP:0004-637X-828-1-14 |
| 出版者 | The American Astronomical Society |
| 源URL | [http://119.78.226.72/handle/331011/32149]  |
| 专题 | 中国科学院上海天文台 |
| 作者单位 | 1.Key Laboratory of Research in Galaxies and Cosmology, Shanghai Astronomical Observatory, Chinese Academy of Sciences, 80 Nandan Road, Shanghai 200030, China; jshen@shao.ac.cn, vpdebattista@gmail.com 2.Jeremiah Horrocks Institute, University of Central Lancashire, Preston, PR1 2HE, UK 3.Sub-department of Astrophysics, Department of Physics, University of Oxford, Denys Wilkinson Building, Keble Road, Oxford OX1 3RH, UK |
| 推荐引用方式 GB/T 7714 | Du,Min,Debattista,Victor P.,Shen,Juntai,et al. KINEMATIC PROPERTIES OF DOUBLE-BARRED GALAXIES: SIMULATIONS VERSUS INTEGRAL-FIELD OBSERVATIONS[J]. The Astrophysical Journal,2016,828(1). |
| APA | Du,Min,Debattista,Victor P.,Shen,Juntai,&Cappellari,Michele.(2016).KINEMATIC PROPERTIES OF DOUBLE-BARRED GALAXIES: SIMULATIONS VERSUS INTEGRAL-FIELD OBSERVATIONS.The Astrophysical Journal,828(1). |
| MLA | Du,Min,et al."KINEMATIC PROPERTIES OF DOUBLE-BARRED GALAXIES: SIMULATIONS VERSUS INTEGRAL-FIELD OBSERVATIONS".The Astrophysical Journal 828.1(2016). |
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来源：上海天文台
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