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A Determination of the Hubble Constant Using Measurements of X-Ray Emission and the Sunyaev-Zeldovich Effect at Millimeter Wavelengths in the Cluster Abell 1835

Mauskopf, P.D.; Ade, P.A.R.; Allen, S.W.; Church, S.E.; Edge, A.C.; Ganga, K.M.; Holzapfel, W.L.; Lange, A.E.; Rownd, B.K.; Philhour, B.J.; Runyan, M.C.

A Determination of the Hubble Constant Using Measurements of X-Ray Emission and the Sunyaev-Zeldovich Effect at Millimeter Wavelengths in the Cluster Abell 1835 Thumbnail


Authors

P.D. Mauskopf

P.A.R. Ade

S.W. Allen

S.E. Church

K.M. Ganga

W.L. Holzapfel

A.E. Lange

B.K. Rownd

B.J. Philhour

M.C. Runyan



Abstract

We present a determination of the Hubble constant and central electron density in the cluster Abell 1835 (z = 0.2523) from measurements of X-ray emission and millimeter-wave observations of the Sunyaev-Zeldovich (S-Z) effect with the Sunyaev-Zeldovich Infrared Experiment (SuZIE) multifrequency array receiver. Abell 1835 is a well studied cluster in the X-ray with a large central cooling flow. Using a combination of data from ROSAT PSPC and HRI images and millimeter wave measurements we fit a King model to the emission from the ionized gas around Abell 1835 with θ0 = 022 ± 002 and β = 0.58 ± 0.02. Assuming the cluster gas to be isothermal with a temperature of 9.8 keV, we find a y-parameter of 4.9 ± 0.6 × 10-4 and a peculiar velocity of 500 ± 1000 km s-1 from measurements at three frequencies, 145, 221, and 279 GHz. Combining the S-Z measurements with X-ray data, we determine a value for the Hubble constant of H0 = 59 km s-1 Mpc-1 and a central electron density for Abell 1835 of ne0 = 5.64 × 10-2 cm-3 assuming a standard cosmology with Ωm = 1 and ΩΛ = 0. The error in the determination of the Hubble constant is dominated by the uncertainty in the temperature of the X-ray emitting cluster gas.

Citation

Mauskopf, P., Ade, P., Allen, S., Church, S., Edge, A., Ganga, K., …Runyan, M. (2000). A Determination of the Hubble Constant Using Measurements of X-Ray Emission and the Sunyaev-Zeldovich Effect at Millimeter Wavelengths in the Cluster Abell 1835. Astrophysical Journal, 538(2), 505-516. https://doi.org/10.1086/309137

Journal Article Type Article
Publication Date Aug 1, 2000
Deposit Date Sep 12, 2013
Publicly Available Date Jan 3, 2014
Journal Astrophysical Journal
Print ISSN 0004-637X
Electronic ISSN 1538-4357
Publisher American Astronomical Society
Peer Reviewed Peer Reviewed
Volume 538
Issue 2
Pages 505-516
DOI https://doi.org/10.1086/309137
Keywords Cosmology, Observations, Distance scale, Galaxies, Clusters, Individual (A1835), Radio continum, X-rays.

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Copyright Statement
© 2000. The American Astronomical Society. All rights reserved. Printed in the U.S.A.





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