SXP 1062, a young Be X-ray binary pulsar with long spin period - implications 
for the neutron star birth spin

Haberl, F.; Sturm, R.; Filipović, M. D.; Pietsch, W.; Crawford, E. J.

doi:10.1051/0004-6361/201118369

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SXP 1062, a young Be X-ray binary pulsar with long spin period - implications for the neutron star birth spin

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Haberl, F.
High Energy Astrophysics, MPI for Extraterrestrial Physics, Max Planck Society;

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Sturm, R.
High Energy Astrophysics, MPI for Extraterrestrial Physics, Max Planck Society;

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Pietsch, W.
High Energy Astrophysics, MPI for Extraterrestrial Physics, Max Planck Society;

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Haberl, F., Sturm, R., Filipović, M. D., Pietsch, W., & Crawford, E. J. (2012). SXP 1062, a young Be X-ray binary pulsar with long spin period - implications for the neutron star birth spin. Astronomy & Astrophysics, 537: L1, pp. 1-5. doi:10.1051/0004-6361/201118369.

Cite as: https://hdl.handle.net/11858/00-001M-0000-000F-8743-5

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