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  Analytical model for non-thermal pressure in galaxy clusters – III. Removing the hydrostatic mass bias

Shi, X., Komatsu, E., Nagai, D., & Lau, E. T. (2016). Analytical model for non-thermal pressure in galaxy clusters – III. Removing the hydrostatic mass bias. Monthly Notices of the Royal Astronomical Society, 455(3), 2936-2944. doi:10.1093/mnras/stv2504.

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Shi, Xun1, Author           
Komatsu, Eiichiro1, Author           
Nagai, Daisuke1, Author           
Lau, Erwin T., Author
Affiliations:
1Physical Cosmology, MPI for Astrophysics, Max Planck Society, ou_2205644              

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Language(s): eng - English
 Dates: 2016-01-21
 Publication Status: Issued
 Pages: -
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 Table of Contents: -
 Rev. Type: Peer
 Identifiers: DOI: 10.1093/mnras/stv2504
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Title: Monthly Notices of the Royal Astronomical Society
  Abbreviation : Mon. Not. Roy. Astron. Soc.
Source Genre: Journal
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Pages: - Volume / Issue: 455 (3) Sequence Number: - Start / End Page: 2936 - 2944 Identifier: ISSN: 0035-8711
ISSN: 1365-8711