The helium white dwarf in two pulsars: Too cool in PSR J0751+1807 and too hot in PSR J1012+5307?

Monthly Notices of the Royal Astronomical Society

Volumn 321, Issue 1, 2001, Pages 71-76

  Ergma, Ene ^a   Sarna, Marek J ^b   Gerškevitš Antipova, Jelena ^a  

^a UNIVERSITY OF TARTU   (Estonia)

^b NICOLAUS COPERNICUS ASTRONOMICAL CENTER   (Poland)

Author keywords

Binaries: close; Binaries: general; Pulsars: individual: PSR J0751+1807; Pulsars: individual: PSR J1012+5307; Stars: chemically peculiar; Stars: mass loss

Indexed keywords

COOLING; COOLING SYSTEMS; HELIUM; HYDROGEN; PULSARS;

BINARIES: CLOSE; BINARIES:GENERAL; COOLING AGE; COOLING HISTORY; PULSAR: INDIVIDUAL: PSR J0751+1807; PULSAR: INDIVIDUAL: PSR J1012+5307; PULSARS:INDIVIDUAL; STARS: CHEMICALLY PECULIAR; STARS: MASS-LOSS;

WHITE DWARFS;

EID: 0041971023     PISSN: 00358711     EISSN: None     Source Type: Journal    
DOI: 10.1046/j.1365-8711.2001.04000.x     Document Type: Article

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