The photospheric magnetic field and coronal structure of HD171488

Marsden, S. C. and Jardine, M. and Donati, J.-F. and Petit, P. and Semel, M. and Carter, B. D. (2007) The photospheric magnetic field and coronal structure of HD171488. Memorie della Societa Astronomica Italiana, 78 . pp. 307-310. ISSN 1824-016X

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Official URL: http://sait.oat.ts.astro.it/MSAIt780207/index.html

Abstract

From spectropolarimetric observations of the young, single early G-dwarf HD 171488, we have used Zeeman Doppler imaging to reconstruct brightness and magnetic maps of the star. The inclusion of a solar-like differential rotation law into the imaging process has enabled the measurement of the star's surface differential rotation from the brightness features. In addition, we have created a coronal structure for HD 171488 based on the surface magnetic field distribution.

Item Type:Article (Commonwealth Reporting Category C)
Additional Information:Journal of the Italian Astronomical Society. Awaiting publisher advice.
Fields of Research (FOR2008):02 Physical Sciences > 0201 Astronomical and Space Sciences > 020110 Stellar Astronomy and Planetary Systems
02 Physical Sciences > 0201 Astronomical and Space Sciences > 020102 Astronomical and Space Instrumentation
Subjects:240000 Physical Sciences > 240100 Astronomical Sciences > 240101 Astronomy and Astrophysics
Socio-Economic Objective (SEO2008):UNSPECIFIED
ID Code:3526
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Deposited On:23 Apr 2008 09:31
Last Modified:11 Jan 2012 15:11

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