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Precision cosmology with H2O megamasers: progress in measuring distances to galaxies in the Hubble flow

Published online by Cambridge University Press:  01 March 2007

J. Braatz ,
L. Greenhill ,
M. Reid ,
J. Condon ,
C. Henkel  and
K.-Y. Lo
J. Braatz
Affiliation:
National Radio Astronomy Observatory, Charlottesville, VA, USA email: jbraatz@nrao.edu
L. Greenhill
Affiliation:
Harvard-Smithsonian Center for Astrophysics, Cambridge, MA, USA
M. Reid
Affiliation:
Harvard-Smithsonian Center for Astrophysics, Cambridge, MA, USA
J. Condon
Affiliation:
National Radio Astronomy Observatory, Charlottesville, VA, USA email: jbraatz@nrao.edu
C. Henkel
Affiliation:
Max-Planck-Institut für Radioastronomie, Bonn, Germany
K.-Y. Lo
Affiliation:
National Radio Astronomy Observatory, Charlottesville, VA, USA email: jbraatz@nrao.edu
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Abstract

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A determination of the Hubble Constant (H0) to better than 3% would be the best complement to cosmic microwave background (CMB) data to constrain the equation of state of Dark Energy. Water vapor megamasers provide perhaps the best opportunity for measuring direct distances to galaxies out to about 200 Mpc. We have formed a team of astronomers in the Megamaser Cosmology Project to pursue the ambitious goal of making a precise measurement of H0 by measuring such distances using the techniques pioneered on the disk maser in NGC 4258 by Herrnstein et al (1999). In recent surveys we have made significant progress identifying new maser systems analogous to that in NGC 4258, but more distant. Once the appropriate candidates are identified, two types of observations are necessary to ultimately measure a distance: single-dish monitoring to measure the acceleration of gas in the disk, and sensitive VLBI imaging in order to measure the angular size of the disk, measure the rotation curve, and model radial displacement of the systemic maser features. We have recently obtained preliminary VLBI maps of the masers in two systems, NGC 6323 and UGC 3789. The maser disks in both galaxies were discovered and monitored with the Green Bank Telescope (GBT) and subsequently imaged with the High Sensitivity Array (VLBA + GBT + Effelsberg). In this contribution we present a map of the maser distribution in one of those systems, NGC 6323. The map demonstrates that pc-scale maser disks as distant as ~ 100 Mpc can be imaged with existing telescopes. Results on UGC 3789 will be presented in a later publication.

Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 3 , Symposium S242: Astrophysical Masers and their Environments , March 2007 , pp. 399 - 401
Copyright
Copyright © International Astronomical Union 2008

References

Braatz, J. A., Henkel, C., Greenhill, L. J., Moran, J. M., & Wilson, A. S. 2004, ApJ, 617, L29CrossRefGoogle Scholar
Herrnstein, J. R., Moran, J. M., Greenhill, L. J., Diamond, P. J., Inoue, M., Nakai, N., Miyoshi, M., Henkel, C., & Riess, A. 1999, Nature 400, 539CrossRefGoogle Scholar
Kondratko, P. T., Greenhill, L. J., & Moran, J. M. 2006, ApJ 652, 136CrossRefGoogle Scholar