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Small-Scale Structure Deduced from X- and γ-ray Timing Measurements

Published online by Cambridge University Press:  13 May 2016

M. Coleman Miller
M. Coleman Miller*
Affiliation:
University of Maryland, Department of Astronomy, College Park, MD, USA

Abstract

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X-ray timing observations of neutron stars and black holes are among the few available probes of ultrastrong magnetic fields, strong gravity, high densities, and the propagation of thermonuclear burning. Here we review the evidence for these effects revealed with data from the Rossi Explorer in the last five years. We also discuss the exciting prospects for making the first quantitative tests of strong-gravity general relativistic predictions with a large-area X-ray timing mission.

Type
Star Formation Regions and Outflow Processes in our Galaxy
Information
Symposium - International Astronomical Union , Volume 205: Galaxies and their Constituents at the Highest Angular Resolutions , 2001 , pp. 244 - 251
Copyright
Copyright © Astronomical Society of the Pacific 2001 

References

Akmal, A., Pandharipande, V. R., & Ravenhall, D. G. 1998, Phys. Rev. C58, 1804.Google Scholar
Bildsten, L. 1995, ApJ, 438, 852.CrossRefGoogle Scholar
Cline, T., et al. 2000, ApJ, 531, 407.CrossRefGoogle Scholar
Erber, T. 1966, Rev. Mod. Phys., 38, 626.CrossRefGoogle Scholar
Ford, E. C. 1999, ApJ, 519, L73.CrossRefGoogle Scholar
Ford, E. C. 2000, ApJ, 535, L119.CrossRefGoogle Scholar
Fryxell, B. A., & Woosley, S. E. 1982, ApJ, 258, 773.Google Scholar
in 't Zand, J. et al. 2000, A&A, submitted.Google Scholar
Joss, P. C. 1978, ApJ, 225, L123.Google Scholar
Kouveliotou, C. et al. 1998, Nature, 393, 235.CrossRefGoogle Scholar
Kouveliotou, C. et al. 1999, ApJ, 510, L115.Google Scholar
Marsden, D., Rothschild, R. E., & Ligenfelter, R. E. 1999, ApJ, 523, L97.Google Scholar
Mazets, E. P., et al. 1979, Nature, 282, 587.Google Scholar
Miller, M. C. 1999, ApJ, 515, L77.CrossRefGoogle Scholar
Miller, M. C. 2000, Astr. Lett. Comm, in press (astro-ph/0007287).Google Scholar
Miller, M. C., Lamb, F. K., & Psaltis, D. 1998, ApJ, 508, 791.Google Scholar
Nowak, M. A., et al. 1997, ApJ, 477, L91.CrossRefGoogle Scholar
Nozakura, T., Ikeuchi, S., & Fujimoto, M. Y. 1984, ApJ, 286, 221.Google Scholar
Stella, L., Vietri, M., & Morsink, S. M. 1999, ApJ, 524, L63.CrossRefGoogle Scholar
Stoeger, W. R. 1980, MNRAS, 190, 715.Google Scholar
Strohmayer, T. E., & Markwardt, C. B. 1999, ApJ, 516, L81.Google Scholar
Strohmayer, T. E., Zhang, W., & Swank, J. H. 1997, ApJ, 487, L77.Google Scholar
Strohmayer, T. E., et al. 1998, ApJ, 503, L147.Google Scholar
Sunyaev, R. A. 1973, Sov. Astr. AJ., 16, 941.Google Scholar
Thompson, C., & Duncan, R. C. 1995, MNRAS, 275, 255.Google Scholar
Thompson, C., & Duncan, R. C. 1996, ApJ, 473, 322.Google Scholar
van der Klis, M. 2000, ARA&A, 38, 717.Google Scholar
van Straaten, S., et al. 2000, ApJ, 540, 1049.CrossRefGoogle Scholar
Weinberg, N., Miller, M. C., & Lamb, D. Q. 2000, ApJ, in press.Google Scholar
Woods, P. M. et al. 1999, ApJ, 519, L139.Google Scholar
Zhang, W., et al. 1998, ApJ, 500, L171.CrossRefGoogle Scholar