Formation of the small magellanic cloud: An ancient major merger as a solution to the kinematical differences between old stars and H I gas

Kenji Bekki; M Chiba

doi:10.1086/589441

Formation of the small magellanic cloud: An ancient major merger as a solution to the kinematical differences between old stars and H I gas

Research output: Contribution to journal › Article › peer-review

Original language	English
Pages (from-to)	L89-L92
Journal	The Astrophysical Journal
Volume	679
Issue number	2008 June 1
DOIs	https://doi.org/10.1086/589441
Publication status	Published - 2008

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10.1086/589441

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title = "Formation of the small magellanic cloud: An ancient major merger as a solution to the kinematical differences between old stars and H I gas",

author = "Kenji Bekki and M Chiba",

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journal = "The Astrophysical Journal",

issn = "0004-637X",

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T1 - Formation of the small magellanic cloud: An ancient major merger as a solution to the kinematical differences between old stars and H I gas

AU - Bekki, Kenji

AU - Chiba, M

PY - 2008

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UR - https://www.scopus.com/pages/publications/62749152715

U2 - 10.1086/589441

DO - 10.1086/589441

M3 - Article

SN - 0004-637X

VL - 679

SP - L89-L92

JO - The Astrophysical Journal

JF - The Astrophysical Journal

IS - 2008 June 1

ER -

Formation of the small magellanic cloud: An ancient major merger as a solution to the kinematical differences between old stars and H I gas

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