Dust in the IGM: pro and contra

Please use this identifier to cite or link to this item: http://hdl.handle.net/2289/4155

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DC Field	Value	Language
dc.contributor.author	Shchekinov, Yuri	-
dc.contributor.author	Nath, Biman B.	-
dc.date.accessioned	2011-08-27T07:41:23Z	-
dc.date.available	2011-08-27T07:41:23Z	-
dc.date.issued	2011-02	-
dc.identifier.citation	Astrophysics and Space Science, 2011, Vol.335, p207	en
dc.identifier.issn	0004-640X	-
dc.identifier.issn	1572-946X (Online)	-
dc.identifier.uri	http://hdl.handle.net/2289/4155	-
dc.description	Restricted Access.	en
dc.description.abstract	Observations of dust grains in the intergalactic medium (IGM) allow us to study an important aspect in the evolution of galaxies. Although it existence had been previously speculated upon, direct evidence of the presence of dust in the intergalactic space has only been available recently. We discuss various issues regarding the presence of dust in the IGM—its sources, transport mechanisms from galaxies into the IGM, its effect on reddening and on cosmological studies.	en
dc.language.iso	en	en
dc.publisher	Springer	en
dc.relation.uri	http://adsabs.harvard.edu/doi/10.1007/s10509-011-0640-y	en
dc.relation.uri	http://dx.doi.org/10.1007/s10509-011-0640-y	en
dc.rights	2011 Springer.	en
dc.subject	Intergalatic medium	en
dc.subject	Dust sources	en
dc.subject	Reddening	en
dc.title	Dust in the IGM: pro and contra	en
dc.type	Article	en
Appears in Collections:	Research Papers (A&A)

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