Evidence for an intermediate-mass black hole in NGC 6624

Perera, B.B.P.; Stappers, B.W.; Lyne, A.G.; Bassa, C.G.; Cognard, I.; Guillemot, L.; Kramer, M.; Theureau, G.; Desvignes, G.

doi:10.1017/S1743921317009346

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Evidence for an intermediate-mass black hole in NGC 6624

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Guillemot, L.
Max Planck Institute for Radio Astronomy, Max Planck Society;

Kramer, M.
Max Planck Institute for Radio Astronomy, Max Planck Society;

Desvignes, G.
Max Planck Institute for Radio Astronomy, Max Planck Society;

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Perera, B., Stappers, B., Lyne, A., Bassa, C., Cognard, I., Guillemot, L., et al. (2018). Evidence for an intermediate-mass black hole in NGC 6624. In P. {Weltevrede}, B. {Perera}, L. {Preston}, & S. {Sanidas} (Eds.), Pulsar Astrophysics the Next Fifty Years (pp. 247-250).

Cite as: https://hdl.handle.net/21.11116/0000-0004-3E7A-F

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