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

Details Analyze and predict VLTI observations: the Role of 2D/3D dust continuum radiative transfer codes Analyze and predict VLTI observations: the Role of 2D/3D dust continuum radiative transfer codes

Oct 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003esasp.539..533p&link_type=abstract

In: Proceedings of the Conference on Towards Other Earths: DARWIN/TPF and the Search for Extrasolar Terrestrial Planets, 22-25 A

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Accretion Disks, Interferometry (Midi), Radiative Transfer

Scientific paper

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.

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