DSpace at EWHA: Supersonic waves of magnetization in dark interstellar molecular clouds

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DC Field	Value	Language
dc.contributor.author	양종만	-
dc.date.accessioned	2016-08-28T11:08:27Z	-
dc.date.available	2016-08-28T11:08:27Z	-
dc.date.issued	2000	-
dc.identifier.issn	0021-3640	-
dc.identifier.other	OAK-455	-
dc.identifier.uri	https://dspace.ewha.ac.kr/handle/2015.oak/218650	-
dc.description.abstract	We suggest that supersonic linewidths inferred from recent measurements of magnetic fields toward the core position in dark interstellar molecular clouds may be due to transverse waves of magnetization propagating in a poorly ionized, magnetically ordered gas-dust medium composed of tiny ferromagnetic dusty grains suspended in a cold gaseous cloud of molecular hydrogen. © 2000 MAIK "Nauka/Interperiodica".	-
dc.language	English	-
dc.title	Supersonic waves of magnetization in dark interstellar molecular clouds	-
dc.type	Article	-
dc.relation.issue	10	-
dc.relation.volume	71	-
dc.relation.index	SCI	-
dc.relation.index	SCIE	-
dc.relation.index	SCOPUS	-
dc.relation.startpage	395	-
dc.relation.lastpage	398	-
dc.relation.journaltitle	JETP Letters	-
dc.identifier.wosid	WOS:000087914800001	-
dc.identifier.scopusid	2-s2.0-0040566816	-
dc.author.google	Yang J.	-
dc.author.google	Bastrukov S.I.	-
dc.contributor.scopusid	양종만(15039320200;8833888100)	-
dc.date.modifydate	20230118100842	-