Radiative Transfer Modelling of Dust in the M22 PN IRAS 18333-2357

dc.contributor.author	Muthumariappan, C
dc.contributor.author	Parthasarathy, M
dc.contributor.author	Ita, Y
dc.date.accessioned	2020-11-10T02:37:54Z
dc.date.available	2020-11-10T02:37:54Z
dc.date.issued	2015-08
dc.identifier.citation	ASP conference series; Vol. 497, pp. 493- 494	en_US
dc.identifier.isbn	978-1-58381-878-7
dc.identifier.uri	http://prints.iiap.res.in/handle/2248/6746
dc.description	restricted access © Astronomical Society of the Pacific http://aspbooks.org/custom/publications/paper/497-0493.html	en_US
dc.description.abstract	We report results from our 1-D radiative transfer modelling of dust in the hydrogen-deficient planetary nebula IRAS 18333-2357 and discuss the properties of classical-grain and very small-grain populations of this PN.	en_US
dc.language.iso	en	en_US
dc.publisher	Astronomical Society of the Pacific	en_US
dc.title	Radiative Transfer Modelling of Dust in the M22 PN IRAS 18333-2357	en_US
dc.type	Book	en_US