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Astronomy and astrophysics (Berlin), ISSN 0004-6361, 2014, Volume 572, pp. 1 - 15
Kepler ultra-high precision photometry of long and continuous observations provides a unique dataset in which surface rotation and variability can be studied for thousands of stars... 
Stars: evolution | Stars: activity | Asteroseismology | Stars: oscillations | Stars: rotation | Stars: solar-type | Physical Sciences | Astronomy & Astrophysics | Science & Technology | Metallicity | Stars | Surface chemistry | Calibration | Age | Photometry | Astronomy | Pulsation | Physics - Solar and Stellar Astrophysics | Physics | Astrophysics
Journal Article
Astronomische Nachrichten, ISSN 0004-6337, 10/2017, Volume 338, Issue 8, pp. 903 - 909
From our sample of spotted late‐type stars showing surface differential rotation, we find that the relationship between the rotation period and the surface shear coefficient α = ΔΩ/Ω... 
stars: late type | stars: imaging | differential rotation | starspots | stars: activity | Physical Sciences | Astronomy & Astrophysics | Science & Technology | Differential rotation | Binary systems | Stellar rotation | Binary stars | Physics - Solar and Stellar Astrophysics
Journal Article
Monthly notices of the Royal Astronomical Society, ISSN 1365-2966, 03/2014, Volume 440, Issue 2, pp. 1649 - 1661
...) and rotational excitation up to J = 39. The line list is computed using the eigenvalues and eigenfunctions of CH4 obtained by variational solution of the Schrodinger equation for the rotation-vibration motion of nuclei employing program... 
Astronomical data bases: miscellaneous | Planets and satellites: atmospheres | Opacity | Stars: low-mass | Molecular data | Physical Sciences | Astronomy & Astrophysics | Science & Technology
Journal Article
The Astrophysical journal, ISSN 1538-4357, 10/2014, Volume 794, Issue 2, pp. 144 - 8
Journal Article
Astronomy and astrophysics (Berlin), ISSN 0004-6361, 2015, Volume 581, p. A15
.... We aim to investigate the role of metallicity and rotation in shaping the evolutionary paths of massive stars and to provide theoretical predictions that can be tested by observations of metal-poor environments. Methods... 
massive | Galaxies | Supergiants | Stars | rotation | dwarf | evolution | Ultraviolet | Physical Sciences | Astronomy & Astrophysics | Science & Technology
Journal Article
Astronomy and astrophysics (Berlin), ISSN 0004-6361, 10/2010, Volume 522, Issue 1, p. A10
.... We study the effects of thermohaline instability and rotation-induced mixing in the 1-4 M-circle dot range at solar metallicity. Methods... 
hydrodynamics | stars: interiors | stars: evolution | instabilities | stars: abundances | stars: rotation | Physical Sciences | Astronomy & Astrophysics | Science & Technology | Physics - Solar and Stellar Astrophysics
Journal Article