Investigating the Potential Dilution of the Metal Content of Hot Gas in Early-Type Galaxies by Accreted Cold Gas

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dc.contributor.author Su, Yuanyuan
dc.contributor.author Irwin, Jimmy A.
dc.date.accessioned 2018-09-12T19:48:59Z
dc.date.available 2018-09-12T19:48:59Z
dc.date.issued 2013-03-20
dc.identifier.citation Su, Y., Irwin, J. (2013): Investigating the Potential Dilution of the Metal Content of Hot Gas in Early-Type Galaxies by Accreted Cold Gas. The Astrophysical Journal, 776(1). en_US
dc.identifier.uri http://ir.ua.edu/handle/123456789/3843
dc.format.mimetype application/pdf en_US
dc.subject galaxies: elliptical and lenticular, cD en_US
dc.subject ISM: abundances en_US
dc.subject ISM: atoms en_US
dc.subject ISM: molecules en_US
dc.subject X-rays: galaxies en_US
dc.subject X-rays: ISM en_US
dc.title Investigating the Potential Dilution of the Metal Content of Hot Gas in Early-Type Galaxies by Accreted Cold Gas en_US
dc.type text en_US


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