Doppler imaging of the young late-type star LO Pegasi (BD+22°4409) in 2003 September
Author:
Publisher
Oxford University Press (OUP)
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://academic.oup.com/mnras/article-pdf/387/1/237/3201389/mnras0387-0237.pdf
Reference24 articles.
1. Deconvolution of high-resolution spectra as a signal-to-noise ratio enhancement method
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3. Modelling dynamos in rapidly rotating late-type stars
4. Polar Magnetic Activity and Spin‐down on the Lower Main Sequence
5. A library of high resolution synthetic stellar spectra from 300 nm to 1.8 ${\rm \mu}$m with solar andα-enhanced composition
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1. Active longitudes and starspot evolution of the young rapidly rotating star USNO-B1.0 1388−0463685 discovered in the Yunnan–Hong Kong survey;Monthly Notices of the Royal Astronomical Society;2022-06-11
2. Photometric Observations of LO Peg in 2017;Astrophysical Bulletin;2018-07
3. Young, active radio stars in the AB Doradus moving group;Astronomy & Astrophysics;2017-06
4. LO Peg: surface differential rotation, flares, and spot-topographic evolution;Monthly Notices of the Royal Astronomical Society;2016-04-15
5. The evolution of surface magnetic fields in young solar-type stars – I. The first 250 Myr;Monthly Notices of the Royal Astronomical Society;2016-01-22
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