Gravitational-wave limits from pulsar timing constrain supermassive black hole evolution.

Shannon, R M; Ravi, V; Coles, W A; Hobbs, G; Keith, M J; Manchester, R N; Wyithe, J S B; Bailes, M; Bhat, N D R; Burke-Spolaor, S; Khoo, J; Levin, Y; Oslowski, S; Sarkissian, J M; van Straten, W; Verbiest, J P W; Wang, J-B

Shannon, R M; Ravi, V; Coles, W A; Hobbs, G; Keith, M J; Manchester, R N; Wyithe, J S B; Bailes, M; Bhat, N D R; Burke-Spolaor, S; Khoo, J; Levin, Y; Oslowski, S; Sarkissian, J M; van Straten, W; Verbiest, J P W; Wang, J-B.

Afiliação

Shannon RM; Commonwealth Scientific and Industrial Research Organisation (CSIRO) Astronomy and Space Science, Australia Telescope National Facility, Post Office Box 76, Epping, New South Wales 1710, Australia.

Science ; 342(6156): 334-7, 2013 Oct 18.

Article em En | MEDLINE | ID: mdl-24136962

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Texto completo: 1 Base de dados: MEDLINE Tipo de estudo: Prognostic_studies Idioma: En Ano de publicação: 2013 Tipo de documento: Article

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Texto completo: 1 Base de dados: MEDLINE Tipo de estudo: Prognostic_studies Idioma: En Ano de publicação: 2013 Tipo de documento: Article