Characterizing the heavy elements in globular cluster M22 and an empirical 
s-process abundance distribution derived from the two stellar groups

Roederer, I. U.; Marino, A. F.; Sneden, C.

doi:10.1088/0004-637X/742/1/37

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Characterizing the heavy elements in globular cluster M22 and an empirical s-process abundance distribution derived from the two stellar groups

Roederer, I. U., Marino, A. F., & Sneden, C. (2011). Characterizing the heavy elements in globular cluster M22 and an empirical s-process abundance distribution derived from the two stellar groups. The Astrophysical Journal, 742(1): 37, pp. 1-16. doi:10.1088/0004-637X/742/1/37.

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Item Permalink: https://hdl.handle.net/11858/00-001M-0000-000F-3A78-B Version Permalink: https://hdl.handle.net/11858/00-001M-0000-000F-3A79-9

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Creators:
Roederer, I. U., Author
Marino, A. F.¹, Author
Sneden, C., Author

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1Stellar Astrophysics, MPI for Astrophysics, Max Planck Society, ou_159882

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Language(s): eng - English

Dates: Date issued: 2011-11-20

Publication Status: Issued

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Rev. Type: Peer

Identifiers: DOI: 10.1088/0004-637X/742/1/37

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Title: The Astrophysical Journal

Abbreviation : Astrophys. J.

Source Genre: Journal

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Pages: - Volume / Issue: 742 (1) Sequence Number: 37 Start / End Page: 1 - 16 Identifier: ISSN: 0004-637x