DYNAMICAL MODELING OF TIDAL STREAMS

被引:101
作者
Bovy, Jo [1 ]
机构
[1] Inst Adv Study, Princeton, NJ 08540 USA
关键词
dark matter; galaxies: interactions; Galaxy: halo; Galaxy: kinematics and dynamics; Galaxy: structure; MISSING SATELLITES; ORBIT MISALIGNMENT; STAR-CLUSTERS; MILKY-WAY; GALAXY; HALO; POTENTIALS; ALGORITHM; PROBES; TAILS;
D O I
10.1088/0004-637X/795/1/95
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
I present a new framework for modeling the dynamics of tidal streams. The framework consists of simple models for the initial action-angle distribution of tidal debris, which can be straightforwardly evolved forward in time. Taking advantage of the essentially one-dimensional nature of tidal streams, the transformation to position-velocity coordinates can be linearized and interpolated near a small number of points along the stream, thus allowing for efficient computations of a stream's properties in observable quantities. I illustrate how to calculate the stream's average location (its "track") in different coordinate systems, how to quickly estimate the dispersion around its track, and how to draw mock stream data. As a generative model, this framework allows one to compute the full probability distribution function and marginalize over or condition it on certain phase-space dimensions as well as convolve it with observational uncertainties. This will be instrumental in proper data analysis of stream data. In addition to providing a computationally efficient practical tool for modeling the dynamics of tidal streams, the action-angle nature of the framework helps elucidate how the observed width of the stream relates to the velocity dispersion or mass of the progenitor, and how the progenitors of "orphan" streams could be located. The practical usefulness of the proposed framework crucially depends on the ability to calculate action-angle variables for any orbit in any gravitational potential. A novel method for calculating actions, frequencies, and angles in any static potential using a single orbit integration is described in the Appendix.
引用
收藏
页数:18
相关论文
共 35 条
[1]  
[Anonymous], APPL STAT, DOI DOI 10.2307/2347565
[2]  
Binney J., 2008, GALACTIC DYNAMICS, VSecond
[3]   Fitting orbits to tidal streams [J].
Binney, James .
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 2008, 386 (01) :L47-L51
[4]   Actions for axisymmetric potentials [J].
Binney, James .
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 2012, 426 (02) :1324-1327
[5]   EXTREME DECONVOLUTION: INFERRING COMPLETE DISTRIBUTION FUNCTIONS FROM NOISY, HETEROGENEOUS AND INCOMPLETE OBSERVATIONS [J].
Bovy, Jo ;
Hogg, David W. ;
Roweis, Sam T. .
ANNALS OF APPLIED STATISTICS, 2011, 5 (2B) :1657-1677
[6]   DARK MATTER SUB-HALO COUNTS VIA STAR STREAM CROSSINGS [J].
Carlberg, R. G. .
ASTROPHYSICAL JOURNAL, 2012, 748 (01)
[7]   A very fast and momentum-conserving tree code [J].
Dehnen, W .
ASTROPHYSICAL JOURNAL, 2000, 536 (01) :L39-L42
[8]   A hierarchical O(N) force calculation algorithm [J].
Dehnen, W .
JOURNAL OF COMPUTATIONAL PHYSICS, 2002, 179 (01) :27-42
[9]   The mechanics of tidal streams [J].
Eyre, Andy ;
Binney, James .
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 2011, 413 (03) :1852-1874
[10]  
Fox M., 2012, THESIS U OXFORD