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MOCASSIN: 3D photoionisation and dust radiative transfer modelling of PNe

Ercolano, B; Barlow, MJ; Storey, PJ; Liu, X-W; (2006) MOCASSIN: 3D photoionisation and dust radiative transfer modelling of PNe. In: Stanghellini, L and Walsh, JR and Douglas, NG, (eds.) Planetary Nebulae Beyond the Milky Way. ESO ASTROPHYSICS SYMPOSIA European Southern Observatory. (pp. pp. 196-198). Springer, Berlin, Heidelberg Green open access

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Abstract

We present the first 3D Monte Carlo photoionisation code to include a fully self-consistent treatment of dust radiative transfer (RT) within the photoionised region. This is the latest development of the recently published pure photoionisation code mocassin (Ercolano et al., 2003a) and it is currently undergoing several benchmarking tests. The preliminary results of these tests are presented. The new code provides the ideal tool for the analysis of dusty ionised regions showing asymmetries and/or density and chemical inhomogeneities

Type: Proceedings paper
Title: MOCASSIN: 3D photoionisation and dust radiative transfer modelling of PNe
Event: Workshop on Planetary Nebulae Beyond the Milky Way
Location: ESO Headquarters, Garching, GERMANY
Dates: 19 May 2004 - 21 May 2004
ISBN: 3-540-31011-8
Open access status: An open access version is available from UCL Discovery
DOI: 10.1007/11604792_27
Publisher version: https://doi.org/10.1007/11604792_27
Language: English
Additional information: This version is the author accepted manuscript. For information on re-use, please refer to the publisher’s terms and conditions.
Keywords: Science & Technology, Physical Sciences, Astronomy & Astrophysics
UCL classification: UCL
UCL > Provost and Vice Provost Offices > UCL BEAMS
UCL > Provost and Vice Provost Offices > UCL BEAMS > Faculty of Maths and Physical Sciences
UCL > Provost and Vice Provost Offices > UCL BEAMS > Faculty of Maths and Physical Sciences > Dept of Physics and Astronomy
URI: https://discovery.ucl.ac.uk/id/eprint/10095575
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