Current perspective on the formation of the double pulsar J0737-3039

Details Current perspective on the formation of the double pulsar J0737-3039 Current perspective on the formation of the double pulsar J0737-3039

Mar 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010newar..54..145d&link_type=abstract

New Astronomy Reviews, Volume 54, Issue 3-6, p. 145-147.

Astronomy and Astrophysics

Astronomy

Scientific paper

We review our current perspective on the formation of the double pulsar J0737-3039. Pulsar J0737-3039B, the second-born pulsar, was formed from a low-mass helium star with pre-supernova mass in the range of 1.5-2.2 M&sun;. The formation was accompanied by a low kick velocity. It is also suggested that pulsar B was born via electron-capture supernova.

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