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Autor:
T J Hutchins, D I Jones
The spin-distribution of accreting neutron stars in low-mass X-ray binary (LMXB) systems shows a concentration of pulsars well below the Keplarian break-up limit. It has been suggested that their spin frequencies may be limited by the emission of gra
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::f06d1b20b499ff80b5e01169db2022f2
https://eprints.soton.ac.uk/476658/
https://eprints.soton.ac.uk/476658/