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  A new method for the asteroseismic determination of the evolutionary state of red-giant stars

Elsworth, Y., Hekker, S., Basu, S., & Davies, G. R. (2017). A new method for the asteroseismic determination of the evolutionary state of red-giant stars. Mon. Not. Roy. Astron. Soc., 466, 3344-3352. doi:10.1093/mnras/stw3288.

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Item Permalink: http://hdl.handle.net/11858/00-001M-0000-002C-C25E-E Version Permalink: http://hdl.handle.net/11858/00-001M-0000-002C-C25F-C
Genre: Journal Article

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 Creators:
Elsworth, Yvonne, Author
Hekker, Saskia1, Author              
Basu, Sarbani, Author
Davies, Guy R., Author
Affiliations:
1Max Planck Research Group in Stellar Ages and Galactic Evolution (SAGE), Max Planck Institute for Solar System Research, Max Planck Society, ou_2265636              

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 MPIS_GROUPS: Research Group SAGE
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 Dates: 2017
 Publication Status: Published in print
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 Rev. Method: Peer
 Identifiers: DOI: 10.1093/mnras/stw3288
BibTex Citekey: Elsworth:2017-020
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Title: Mon. Not. Roy. Astron. Soc.
Source Genre: Journal
 Creator(s):
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Publ. Info: -
Pages: - Volume / Issue: 466 Sequence Number: - Start / End Page: 3344 - 3352 Identifier: -