The relation between white dwarf mass and orbital period for binary millisecond radio pulsars orbital period 1 ≤ Porb ≤ 20 days

Astronomy and Astrophysics

Volumn 315, Issue 1, 1996, Pages

  Ergma, Ene ^a,b  

^a UNIVERSITY OF TARTU   (Estonia)

^b NORDITA   (Denmark)

Author keywords

Binaries: close stars: evolution; Stars: Mwd Porb relation, MSBP

Indexed keywords

EID: 0043196726     PISSN: 00046361     EISSN: None     Source Type: Journal    
DOI: None     Document Type: Article

References (9)

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