Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/5023
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dc.contributor.authorShah, G. A-
dc.contributor.authorKrishna Swamy, K. S-
dc.date.accessioned2010-02-19T12:46:00Z-
dc.date.available2010-02-19T12:46:00Z-
dc.date.issued1979-11-
dc.identifier.citationKodaikanal Observatory Bulletins Series A, Vol. 2, No. 3, pp. 195 – 202en
dc.identifier.issn0374-3632-
dc.identifier.urihttp://hdl.handle.net/2248/5023-
dc.description.abstractSimple models of the reflection nebula in the form of homogeneous plane-parallel slab containing single scattering silicate and graphite grains taken one species at a time have been considered in view of the far-ultraviolet surface brightness observations obtained from the ANS satellite. The colour difference between the star and the nebula as well the polarization of the nebular light in the far-ultraviolet have also been givenen
dc.language.isoenen
dc.publisherIndian Institute of Astrophysicsen
dc.rights© Indian Institute of Astrophysicsen
dc.subjectReflection Nebulaeen
dc.subjectInterstellar Grainsen
dc.subjectReflection Nebulae:Modelsen
dc.subjectReflection Nebulae:UV Radiationen
dc.subjectFar-Ultraviolet Colours and Photonsen
dc.titleReflection nebula in the far-ultraviolet. 2. Silicate and graphite grainsen
dc.typeArticleen
Appears in Collections:IIAP Publications
Kodaikanal Observatory Bulletins (1905 - 1997 )

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