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 . The formation was accompanied by a low kick velocity. It is also suggested that p
β¦ LIBER β¦
Prospects for measuring the moment of inertia of pulsar J0737-3039A
β Scribed by Lorenzo Iorio
- Publisher
- Elsevier Science
- Year
- 2009
- Tongue
- English
- Weight
- 158 KB
- Volume
- 14
- Category
- Article
- ISSN
- 1384-1076
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