Analyze and predict VLTI observations: The role of 2D/3D dust continuum radiative transfer codes

被引：0
|
作者：
Pascucci, I [1 ]
Henning, T [1 ]
Steinacker, J [1 ]
Wolf, S [1 ]
机构：
[1] Max Planck Inst Astron, D-69117 Heidelberg, Germany
来源：
TOWARDS OTHER EARTHS: DARWIN/TPF AND THE SEARCH FOR EXTRASOLAR TERRESTRIAL PLANETS, PROCEEDINGS | 2003年 / 539卷
关键词：
accretion disks; interferometry (MIDI); radiative transfer;
D O I：
暂无
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
Radiative Transfer (RT) codes with image capability are a fundamental tool for preparing interferometric observations and for interpreting visibility data. In view of the upcoming VLTI facilities, we present the first comparison of images/visibilities coming from two 3D codes that use completely different techniques to solve the problem of self-consistent continuum RT. In addition, we focus on the astrophysical case of a disk distorted by tidal interaction with by-passing stars or internal planets and investigate for which parameters the distortion can be best detected in the mid-infrared using the mid-infrared interferometric device MIDI.
引用
收藏
页码：533 / 536
页数：4
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