Timing of millisecond pulsars in NGC 6752: Evidence for a high mass-to-light ratio in the cluster core

Astrophysical Journal

Volumn 570, Issue 2 II, 2002, Pages

  D'Amico, N ^a,b   Possenti, A ^a   Fici, L ^c   Manchester, R N ^d   Lyne, A G ^e   Camilo, F ^f   Sarkissian, J ^d  

^a INAF OSSERVATORIO ASTRONOMICO DI BOLOGNA   (Italy)

^b INAF OSSERVATORIO ASTRONOMICO DI CAGLIARI   (Italy)

^c UNIVERSITY OF BOLOGNA   (Italy)

^d CSIRO   (Australia)

^e UNIVERSITY OF MANCHESTER   (United Kingdom)

^f Och Spine at New York Presbyterian Hospitals   (United States)

Author keywords

Globular clusters: individual (NGC 6752); Pulsars: individual (PSR J1910 5959B, PSR J1910 5959D, PSR J1910 5959E, PSR J1911 5958A, PSR J1911 6000C)

Indexed keywords

EID: 0012448686     PISSN: 0004637X     EISSN: 15384357     Source Type: Journal    
DOI: 10.1086/341030     Document Type: Article

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