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
Metadata
| HTML Citation | EndNote | Dublin Core | Reference Manager |
Full text not available from this archive.
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 |
| Deposited By: | |
| Deposited On: | 23 Apr 2008 09:31 |
| Last Modified: | 11 Jan 2012 15:11 |
Archive Staff Only: edit this record
