Reflection nebula in the far-ultraviolet. 2. Silicate and graphite grains

dc.contributor.author	Shah, G. A
dc.contributor.author	Krishna Swamy, K. S
dc.date.accessioned	2010-02-19T12:46:00Z
dc.date.available	2010-02-19T12:46:00Z
dc.date.issued	1979-11
dc.identifier.citation	Kodaikanal Observatory Bulletins Series A, Vol. 2, No. 3, pp. 195 – 202	en
dc.identifier.issn	0374-3632
dc.identifier.uri	http://hdl.handle.net/2248/5023
dc.description.abstract	Simple 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 given	en
dc.language.iso	en	en
dc.publisher	Indian Institute of Astrophysics	en
dc.rights	© Indian Institute of Astrophysics	en
dc.subject	Reflection Nebulae	en
dc.subject	Interstellar Grains	en
dc.subject	Reflection Nebulae:Models	en
dc.subject	Reflection Nebulae:UV Radiation	en
dc.subject	Far-Ultraviolet Colours and Photons	en
dc.title	Reflection nebula in the far-ultraviolet. 2. Silicate and graphite grains	en
dc.type	Article	en