Can we predict the magnetic properties of PMS stars from their H-R diagram location?

S. G. Gregory; J. -F. Donati; J. Morin; G. A. J. Hussain; N. J. Mayne; L. A. Hillenbrand; M. Jardine

doi:10.1017/S1743921314001677

Can we predict the magnetic properties of PMS stars from their H-R diagram location?

S. G. Gregory, J. -F. Donati, J. Morin, G. A. J. Hussain, N. J. Mayne, L. A. Hillenbrand, M. Jardine

Research output: Chapter in Book/Report/Conference proceeding › Conference contribution

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....

Original language	English
Title of host publication	Proceedings of the International Astronomical Union
Subtitle of host publication	Magnetic Fields throughout Stellar Evolution
Editors	Pascal Petit, Moira Jardine, Hendrik Spruit
Publisher	Cambridge University Press
Volume	9
Edition	s302
DOIs	https://doi.org/10.1017/S1743921314001677
Publication status	Published - Aug 2014

ASJC Scopus subject areas

Astronomy and Astrophysics

Access to Document

10.1017/S1743921314001677

Cite this

Gregory, S. G., Donati, J. .-F., Morin, J., Hussain, G. A. J., Mayne, N. J., Hillenbrand, L. A., & Jardine, M. (2014). Can we predict the magnetic properties of PMS stars from their H-R diagram location? In P. Petit, M. Jardine, & H. Spruit (Eds.), Proceedings of the International Astronomical Union: Magnetic Fields throughout Stellar Evolution (s302 ed., Vol. 9). Cambridge University Press. https://doi.org/10.1017/S1743921314001677

@inproceedings{f35ae0903dc64dd0b0d379a284d394e7,

title = "Can we predict the magnetic properties of PMS stars from their H-R diagram location?",

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....",

author = "Gregory, {S. G.} and Donati, {J. -F.} and J. Morin and Hussain, {G. A. J.} and Mayne, {N. J.} and Hillenbrand, {L. A.} and M. Jardine",

year = "2014",

month = aug,

doi = "10.1017/S1743921314001677",

language = "English",

volume = "9",

editor = "Pascal Petit and Moira Jardine and Hendrik Spruit",

booktitle = "Proceedings of the International Astronomical Union",

publisher = "Cambridge University Press",

address = "United Kingdom",

edition = "s302",

}

Gregory, SG, Donati, J-F, Morin, J, Hussain, GAJ, Mayne, NJ, Hillenbrand, LA & Jardine, M 2014, Can we predict the magnetic properties of PMS stars from their H-R diagram location? in P Petit, M Jardine & H Spruit (eds), Proceedings of the International Astronomical Union: Magnetic Fields throughout Stellar Evolution. s302 edn, vol. 9, Cambridge University Press. https://doi.org/10.1017/S1743921314001677

Can we predict the magnetic properties of PMS stars from their H-R diagram location? / Gregory, S. G.; Donati, J. -F.; Morin, J. et al.
Proceedings of the International Astronomical Union: Magnetic Fields throughout Stellar Evolution. ed. / Pascal Petit; Moira Jardine; Hendrik Spruit. Vol. 9 s302. ed. Cambridge University Press, 2014.

Research output: Chapter in Book/Report/Conference proceeding › Conference contribution