The Mass Loss Return from Evolved Stars to the Large Magellanic Cloud: Empirical Relations for Excess Emission at 8 and 24 u}m

請用此 Handle URI 來引用此文件： http://ir.sinica.edu.tw/handle/201000000A/53620

題名:	The Mass Loss Return from Evolved Stars to the Large Magellanic Cloud: Empirical Relations for Excess Emission at 8 and 24 u}m
作者:	S. Srinivasan M. Meixner C. Leitherer U. Vijh K. Volk R. D. Blum B. L. Babler M. Block S. Bracker M. Cohen C. W. Engelbracht B.-Q. For K. D. Gordon J. Harris J. L. Hora R. Indebetouw F. Markwick-Kemper M. Meade K. A. Misselt M. Sewilo B. Whitney
公開日期:	2009-06
關聯:	ASTRONOMICAL JOURNAL 137, 4810-4823
URI:	http://ir.sinica.edu.tw/handle/201000000A/53620
ISSN:	http://gateway.isiknowledge.com/gateway/Gateway.cgi?GWVersion=2&SrcAuth=Drexel&SrcApp=hagerty_opac&KeyRecord=0004-6256&DestApp=JCR&RQ=IF_CAT_BOXPLOT
顯示於：	天文及天文物理研究所

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