Reflection Nebula in the Far Ultraviolet: Icy Grains

Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/79

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DC Field	Value	Language
dc.contributor.author	Shah, G. A	-
dc.contributor.author	Krishna Swamy, K. S	-
dc.date.accessioned	2004-12-01T07:10:52Z	-
dc.date.available	2004-12-01T07:10:52Z	-
dc.date.issued	1978	-
dc.identifier.citation	Kodaikanal Observatory Bulletins Series A, Vol. 2, pp. 95-104	en
dc.identifier.issn	0374-3632	-
dc.identifier.uri	http://hdl.handle.net/2248/79	-
dc.description.abstract	Some models of the reflection nebula in the form of homogeneous plane parallel slab containing singly scattering dirty ice grains as test case have been given. The three geometric cases of the star behind, within and in front of the nebula have been considered. The size distribution of the grains has also been incorporated. We have calculated the nebular surface brightness and band integrated colours and polarization. The present results on the nebular surface brightness have been directly compared with the very recent far-ultraviolet observations of the Merope reflection nebula.	en
dc.format.extent	362993 bytes	-
dc.format.mimetype	application/pdf	-
dc.language.iso	en	-
dc.publisher	Indian Institute of Astrophysics, Bangalore	en
dc.subject	Reflection Nebula	en
dc.subject	Interstellar Grains	en
dc.subject	Far Ultraviolet Colours and Polarization	en
dc.title	Reflection Nebula in the Far Ultraviolet: Icy Grains	en
dc.type	Article	en
Appears in Collections:	IIAP Publications Kodaikanal Observatory Bulletins (1905 - 1997 )

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