Files in this item
Activity and magnetic field structure of the Sun-like planet-hosting star HD 1237
Item metadata
dc.contributor.author | Alvarado-Gómez, J.D. | |
dc.contributor.author | Hussain, Gaitee Ara Jaffer | |
dc.contributor.author | Grunhut, J. | |
dc.contributor.author | Fares, Rim | |
dc.contributor.author | Donati, J.-F. | |
dc.contributor.author | Alecian, E. | |
dc.contributor.author | Kochukhov, O. | |
dc.contributor.author | Oksala, M. | |
dc.contributor.author | Morin, J. | |
dc.contributor.author | Redfield, S. | |
dc.contributor.author | Cohen, O. | |
dc.contributor.author | Drake, J.J. | |
dc.contributor.author | Jardine, Moira Mary | |
dc.contributor.author | Matt, S. | |
dc.contributor.author | Petit, P. | |
dc.contributor.author | Walter, F.M. | |
dc.date.accessioned | 2015-11-05T14:10:05Z | |
dc.date.available | 2015-11-05T14:10:05Z | |
dc.date.issued | 2015-10 | |
dc.identifier.citation | Alvarado-Gómez , J D , Hussain , G A J , Grunhut , J , Fares , R , Donati , J-F , Alecian , E , Kochukhov , O , Oksala , M , Morin , J , Redfield , S , Cohen , O , Drake , J J , Jardine , M M , Matt , S , Petit , P & Walter , F M 2015 , ' Activity and magnetic field structure of the Sun-like planet-hosting star HD 1237 ' , Astronomy & Astrophysics , vol. 582 . https://doi.org/10.1051/0004-6361/201525771 | en |
dc.identifier.issn | 0004-6361 | |
dc.identifier.other | PURE: 228687733 | |
dc.identifier.other | PURE UUID: d4ae4edb-e5ed-4cf2-8109-fe7bdc0a6b67 | |
dc.identifier.other | Scopus: 84943158140 | |
dc.identifier.other | WOS: 000363538500038 | |
dc.identifier.other | ORCID: /0000-0002-1466-5236/work/57821904 | |
dc.identifier.uri | https://hdl.handle.net/10023/7744 | |
dc.description | Date of Acceptance: 13/07/2015 | en |
dc.description.abstract | We analyse the magnetic activity characteristics of the planet-hosting Sun-like star, HD 1237, using HARPS spectro-polarimetric time-series data. We find evidence of rotational modulation of the magnetic longitudinal field measurements that is consistent with our ZDI analysis with a period of 7 days. We investigate the effect of customising the LSD mask to the line depths of the observed spectrum and find that it has a minimal effect on the shape of the extracted Stokes V profile but does result in a small increase in the S/N (~7%). We find that using a Milne-Eddington solution to describe the local line profile provides a better fit to the LSD profiles in this slowly rotating star, which also affects the recovered ZDI field distribution. We also introduce a fit-stopping criterion based on the information content (entropy) of the ZDI map solution set. The recovered magnetic field maps show a strong (+90 G) ring-like azimuthal field distribution and a complex radial field dominating at mid latitudes (~45 degrees). Similar magnetic field maps are recovered from data acquired five months apart. Future work will investigate how this surface magnetic field distribution affects the coronal magnetic field and extended environment around this planet-hosting star. | |
dc.language.iso | eng | |
dc.relation.ispartof | Astronomy & Astrophysics | en |
dc.rights | © ESO, 2015. Reproduced with permission from Astronomy & Astrophysics, © ESO. This is the final published version of the work, which was originally published at: http://dx.doi.org/10.1051/0004-6361/201525771 | en |
dc.subject | Stars: activity | en |
dc.subject | Stars: magnetic field | en |
dc.subject | Stars: solar-type | en |
dc.subject | Stars: individual: HD 1237 | en |
dc.subject | QC Physics | en |
dc.subject | QB Astronomy | en |
dc.subject | NDAS | en |
dc.subject.lcc | QC | en |
dc.subject.lcc | QB | en |
dc.title | Activity and magnetic field structure of the Sun-like planet-hosting star HD 1237 | en |
dc.type | Journal article | en |
dc.contributor.sponsor | Science & Technology Facilities Council | en |
dc.contributor.sponsor | Science & Technology Facilities Council | en |
dc.description.version | Publisher PDF | en |
dc.contributor.institution | University of St Andrews. School of Physics and Astronomy | en |
dc.identifier.doi | https://doi.org/10.1051/0004-6361/201525771 | |
dc.description.status | Peer reviewed | en |
dc.identifier.grantnumber | ST/M001296/1 | en |
dc.identifier.grantnumber | ST/J001651/1 | en |
This item appears in the following Collection(s)
Items in the St Andrews Research Repository are protected by copyright, with all rights reserved, unless otherwise indicated.