%0 Generic %1 citeulike:12685886 %A Gregory, S. G. %A Donati, J. F. %A Morin, J. %A Hussain, G. A. J. %A Mayne, N. J. %A Hillenbrand, L. A. %A Jardine, M. %D 2013 %K imported %T Can we predict the magnetic properties of PMS stars from their H-R diagram location? %U http://arxiv.org/abs/1309.7556 %X Spectropolarimetric observations combined with tomographic imaging techniques have revealed that all pre-main sequence (PMS) stars host multipolar magnetic fields, ranging from strong and globally axisymmetric with \~>kilo-Gauss dipole components, to complex and non-axisymmetric with weak dipole components (<\~0.1 kG). Many host dominantly octupolar large-scale fields. We argue that the large-scale magnetic properties of a PMS star are related to its location in the Hertzsprung-Russell diagram. This conference paper is a synopsis of Gregory et al. (2012), updated to include the latest results from magnetic mapping studies of PMS stars.

@misc{citeulike:12685886, abstract = {{Spectropolarimetric observations combined with tomographic imaging techniques have revealed that all pre-main sequence (PMS) stars host multipolar magnetic fields, ranging from strong and globally axisymmetric with \~{}\>kilo-Gauss dipole components, to complex and non-axisymmetric with weak dipole components (\<\~{}0.1 kG). Many host dominantly octupolar large-scale fields. We argue that the large-scale magnetic properties of a PMS star are related to its location in the Hertzsprung-Russell diagram. This conference paper is a synopsis of Gregory et al. (2012), updated to include the latest results from magnetic mapping studies of PMS stars.}}, added-at = {2019-03-25T08:20:55.000+0100}, archiveprefix = {arXiv}, author = {Gregory, S. G. and Donati, J. F. and Morin, J. and Hussain, G. A. J. and Mayne, N. J. and Hillenbrand, L. A. and Jardine, M.}, biburl = {https://www.bibsonomy.org/bibtex/286d5385ba91d50f35bd98e3d6eda3d4b/ericblackman}, citeulike-article-id = {12685886}, citeulike-linkout-0 = {http://arxiv.org/abs/1309.7556}, citeulike-linkout-1 = {http://arxiv.org/pdf/1309.7556}, day = 29, eprint = {1309.7556}, interhash = {2586c0df740951b0068ba580870efbc0}, intrahash = {86d5385ba91d50f35bd98e3d6eda3d4b}, keywords = {imported}, month = sep, posted-at = {2013-10-03 05:43:03}, priority = {2}, timestamp = {2019-03-25T08:20:55.000+0100}, title = {{Can we predict the magnetic properties of PMS stars from their H-R diagram location?}}, url = {http://arxiv.org/abs/1309.7556}, year = 2013 }