Implications of a VLBI distance to the double pulsar J0737-3039A/B

Science

Volumn 323, Issue 5919, 2009, Pages 1327-1329

  Deller, A T ^a   Bailes, M ^a   Tingay, S J ^b  

^a SWINBURNE UNIVERSITY OF TECHNOLOGY   (Australia)

^b CURTIN UNIVERSITY   (Australia)

Author keywords

[No Author keywords available]

Indexed keywords

ACCURACY ASSESSMENT; GRAVITY FIELD; INTERFEROMETRY;

ARTICLE; GRAVITY; INTERFEROMETRY; INTROSPECTION; OBSERVATIONAL STUDY; PREDICTION; PRIORITY JOURNAL; RADIATION; THEORY; VELOCITY;

EID: 62149088105     PISSN: 00368075     EISSN: 10959203     Source Type: Journal    
DOI: 10.1126/science.1167969     Document Type: Article

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29. We acknowledge discussions with M. Kramer and E. van den Heuvel. A.T.D. is supported via a Swinburne University of Technology Chancellor's Research Scholarship and a Commonwealth Scientific and Industrial Research Organisation (CSIRO) postgraduate scholarship. The Long Baseline Array is part of the Australia Telescope, which is funded by the Commonwealth of Australia for operation as a National Facility managed by CSIRO.