1.
Adv Space Biol Med
; 4: 189-224, 1994.
Artigo
em Inglês
| MEDLINE
| ID: mdl-7757251
2.
Astron Astrophys
; 161: 303-4, 1986.
Artigo
em Inglês
| MEDLINE
| ID: mdl-11542034
RESUMO
On July 7, 1984 pulsar 0656+14 was found to exhibit a larger period than expected. Using observations from a number of sources, we have attempted to explain this discrepancy. No indications of orbital motion was found. The available evidence indicates that the star has a period derivative of 54 10(-15) s s-1 rather than 1.6 10(-15) s s-1 as previously reported.
