Proper motion of binary pulsars as a source of secular variations of orbital parameters

Astrophysical Journal

Volumn 467, Issue 2 PART II, 1996, Pages

  Kopeikin, S M ^a,b  

^a NATIONAL ASTRONOMICAL OBSERVATORY OF JAPAN   (Japan)

^b LEBEDEV PHYSICAL INSTITUTE   (Russian Federation)

Author keywords

Gravitation; Relativity; Stars: binaries; Stars: fundamental parameters; Stars: neutron

Indexed keywords

EID: 15444365159     PISSN: 0004637X     EISSN: 15384357     Source Type: Journal    
DOI: 10.1086/310201     Document Type: Article

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