A class of black holes of intermediate mass is expected but has never been detected. The suggestion that these beasts might lurk behind powerful X-ray sources in nearby galaxies is now strengthened.
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References
Ghez, A. M., Morris, M., Becklin, E. E., Tanner, A. & Kremenek, T. Nature 407, 349–351 (2000).
Portegies Zwart, S. F., Baumgardt, H., Hut, P., Makino, J. & McMillan, S. L. W. Nature 428, 724–726 (2004).
Kaaret, P. et al. Mon. Not. R. Astron. Soc. 348, L28–L32 (2004).
Fabbiano, G., Zezas, A. & Murray, S. S. Astrophys. J. 554, 1035–1043 (2001).
van der Marel, R. P. in Coevolution of Black Holes and Galaxies (ed. Ho, L. C.) (Cambridge Univ. Press, in the press).
Gurkan, M. A., Freitag, M. & Rasio, F. A. Astrophys. J. 604, 632–652 (2004).
Bonnell, I. A. & Bate, M. R. Mon. Not. R. Astron. Soc. 336, 659–669 (2002).
McCrady, N., Gilbert, A. M. & Graham, J. R. Astrophys J. 597, 240–252 (2003).
Kaaret, P. et al. Mon. Not. R. Astron. Soc. 321, L29–L31 (2001).
King, A. R., Davies, M. B., Ward, M. J., Fabbiano, G. & Elvis, M. Astrophys. J. 552, L109–L112 (2001).
Begelman, M. C. Astrophys. J. 551, 897–906 (2001).
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McCrady, N. The missing black-hole link. Nature 428, 704–705 (2004). https://doi.org/10.1038/428704a
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DOI: https://doi.org/10.1038/428704a