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  Evidence for an intermediate-mass black hole in NGC 6624

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).

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 Creators:
Perera, B.B.P., Author
Stappers, B.W., Author
Lyne, A.G., Author
Bassa, C.G., Author
Cognard, I., Author
Guillemot, L.1, Author
Kramer, M.1, Author
Theureau, G., Author
Desvignes, G.1, Author
Affiliations:
1Max Planck Institute for Radio Astronomy, Max Planck Society, ou_2205652              

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Free keywords: black hole physics-stars: neutron-pulsars: individual: PSR B1820-30A-globular clusters: individual: NGC 6624
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 Dates: 2018-08
 Publication Status: Issued
 Pages: -
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 Rev. Type: -
 Identifiers: DOI: 10.1017/S1743921317009346
BibTex Citekey: 2018iaus..337..247p
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Title: Pulsar Astrophysics the Next Fifty Years
Source Genre: Proceedings
 Creator(s):
{Weltevrede}, P., Editor
{Perera}, B.~B.~P., Editor
{Preston}, L.~L., Editor
{Sanidas}, S., Editor
Affiliations:
-
Publ. Info: -
Pages: - Volume / Issue: 337 Sequence Number: - Start / End Page: 247 - 250 Identifier: -

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Title: IAU Symposium
Source Genre: Series
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Pages: - Volume / Issue: - Sequence Number: - Start / End Page: - Identifier: -