Flattening modulus of a neutron star by rotation and magnetic field Export

@misc{konno2000, abstract = {We calculated the ellipticity of the deformed star due to the rotation or magnetic field. These two effects are compared to each other within general relativity. It turned out that the magnetic distortion is important for recently observed candidates of magnetars, while the magnetic effect can be neglected for well-known typical pulsars.}, archivePrefix = {arXiv}, author = {Konno, K. and Obata, T. and Kojima, Y.}, citeulike-article-id = {2816783}, citeulike-linkout-0 = {http://arxiv.org/abs/astro-ph/0001397}, citeulike-linkout-1 = {http://arxiv.org/pdf/astro-ph/0001397}, day = {22}, eprint = {astro-ph/0001397}, keywords = {analytical, fields, magnetic, methods, neutron, relativity, rotation, stars}, month = {Jan}, posted-at = {2008-05-20 16:16:14}, priority = {0}, title = {Flattening modulus of a neutron star by rotation and magnetic field}, url = {http://arxiv.org/abs/astro-ph/0001397}, year = {2000} }

TY - ELEC ID - konno2000 L3 - citeulike-article-id:2816783 N2 - We calculated the ellipticity of the deformed star due to the rotation or magnetic field. These two effects are compared to each other within general relativity. It turned out that the magnetic distortion is important for recently observed candidates of magnetars, while the magnetic effect can be neglected for well-known typical pulsars. TI - Flattening modulus of a neutron star by rotation and magnetic field KW - analytical KW - fields KW - magnetic KW - methods KW - neutron KW - relativity KW - rotation KW - stars AU - Konno, K AU - Obata, T AU - Kojima, Y PY - 2000/Jan/22/ UR - http://arxiv.org/abs/astro-ph/0001397 ER -