Magnetic fields and differential rotation on the pre-main sequence - I. The early-G star HD 141943 - brightness and magnetic topologies-Reference-Cited by-同舟云学术

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Magnetic fields and differential rotation on the pre-main sequence - I. The early-G star HD 141943 - brightness and magnetic topologies

Published:2011-04-01 Issue:3 Volume:413 Page:1922-1938
ISSN:0035-8711
Container-title:Monthly Notices of the Royal Astronomical Society
language:en
Short-container-title:

Author:

Marsden S. C.,Jardine M. M.,Ramírez Vélez J. C.,Alecian E.,Brown C. J.,Carter B. D.,Donati J.-F.,Dunstone N.,Hart R.,Semel M.,Waite I. A.

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://academic.oup.com/mnras/article-pdf/413/3/1922/2890861/mnras0413-1922.pdf

Reference64 articles.

1. Chromospheric variations in main-sequence stars

2. The highly spotted photosphere of the young rapid rotator Speedy Mic

3. Doppler images from dual-site observations of southern rapidly rotating stars -- I. Differential rotation on PZ Tel

4. Doppler images from dual-site observations of southern rapidly rotating stars - II. Starspot patterns and differential rotation on Speedy Mic

5. Further images of Persei G dwarfs

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