DISCOVERY OF A 1.6 YEAR MAGNETIC ACTIVITY CYCLE IN THE EXOPLANET HOST STAR ι HOROLOGII-Reference-Cited by-同舟云学术

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DISCOVERY OF A 1.6 YEAR MAGNETIC ACTIVITY CYCLE IN THE EXOPLANET HOST STAR ι HOROLOGII

Published:2010-10-18 Issue:2 Volume:723 Page:L213-L217
ISSN:2041-8205
Container-title:The Astrophysical Journal
language:
Short-container-title:ApJ

Author:

Metcalfe T. S.,Basu S.,Henry T. J.,Soderblom D. R.,Judge P. G.,Knölker M.,Mathur S.,Rempel M.

Publisher

American Astronomical Society

Subject

Space and Planetary Science,Astronomy and Astrophysics

Reference45 articles.

1. CoRoT sounds the stars: p-mode parameters of Sun-like oscillations on HD 49933

2. Chromospheric variations in main-sequence stars

3. On deriving p-mode parameters for inclined solar-like stars

4. PHOTOMETRIC VARIABILITY IN KEPLER TARGET STARS: THE SUN AMONG STARS—A FIRST LOOK

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1. Magnetic activity variability of nearby bright Sun-like stars by 4 yr intensive Hα line monitoring;Publications of the Astronomical Society of Japan;2023-12-04

2. Stellar activity and differential rotation of HD 111395;Astronomy & Astrophysics;2023-12-04

3. Stellar Activity Cycles;Space Science Reviews;2023-09-28

4. Variability of Known Exoplanet Host Stars Observed by TESS;The Astronomical Journal;2023-07-20

5. Far beyond the Sun − II. Probing the stellar magnetism of the young Sun ι Horologii from the photosphere to its corona;Monthly Notices of the Royal Astronomical Society;2023-07-13

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