Accurate mass ratio and heating effects in the dual-line millisecond binary pulsar in NGC 6397

Astrophysical Journal

Volumn 584, Issue 1 II, 2003, Pages

  Ferraro, F R ^a   Sabbi, E ^a   Gratton, R ^b   Possenti, A ^c   D'Amico, N ^c,d   Bragaglia, A ^e   Camilo, F ^f  

^a UNIVERSITY OF BOLOGNA   (Italy)

^b INAF OSSERVATORIO ASTRONOMICO DI PADOVA   (Italy)

^c INAF OSSERVATORIO ASTRONOMICO DI CAGLIARI   (Italy)

^d UNIVERSITY OF CAGLIARI   (Italy)

^e OSSERVATORIO ASTRONOMICO DI BOLOGNA   (Italy)

^f Howard Hughes Medical Institute   (United States)

Author keywords

Binaies: close; Globular clusters: individual (NGC 6397); Pulsars: individual (PSR J1740 5340); Stars: evolution; Techniques: spectroscopic

Indexed keywords

EID: 0041759882     PISSN: 0004637X     EISSN: 15384357     Source Type: Journal    
DOI: 10.1086/368279     Document Type: Article

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