1 | Pulsar astronomers usually define the luminosity ![]() ![]() ![]() ![]() |
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2 | The likely DNS binary J1756![]() ![]() ![]() |
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3 | It is likely, however, that a more detailed statistical analysis of the data are required to confirm or refute this result [82]. |
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http://www.livingreviews.org/lrr-2005-7 |
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