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

Elsworth, Yvonne; Hekker, Saskia; Basu, Sarbani; Davies, Guy R.

doi:10.1093/mnras/stw3288

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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: https://hdl.handle.net/11858/00-001M-0000-002C-C25E-E Version Permalink: https://hdl.handle.net/11858/00-001M-0000-002C-C25F-C

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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: Date issued: 2017

Publication Status: Issued

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Rev. Type: 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

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Pages: - Volume / Issue: 466 Sequence Number: - Start / End Page: 3344 - 3352 Identifier: -