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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 | DWARFS | MAGNETIC-FIELDS | PATTERNS | PRE-MAIN-SEQUENCE | FLOW | SPOT EVOLUTION | KEPLER STARS | ASTRONOMY & ASTROPHYSICS | SUBGIANT | GIANT STARS | COOL ACTIVE STARS | 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, 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 | planets and satellites: atmospheres | EXOPLANET | DIPOLE-MOMENT SURFACES | ROVIBRATIONAL ENERGIES | HIGH-TEMPERATURE | BAND | HOT METHANE | 1ST PRINCIPLES | ATMOSPHERES | BROWN DWARF | molecular data | ASTRONOMY & ASTROPHYSICS | stars: low-mass | opacity | MOLECULAR SPECTROSCOPIC DATABASE | astronomical data bases: miscellaneous
Journal Article
The Astrophysical journal, ISSN 1538-4357, 2014, Volume 794, Issue 2, pp. 144 - 8
Journal Article
2009, 1. Aufl., ISBN 3527407804, xxii, 351
Filling the need for a book that conveys the current technology as well as the underlying history and physical background, this book tells physicists and... 
Earth | Time | Time measurements | Rotation
Book
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 | PRESUPERNOVA EVOLUTION | stars: evolution | B-TYPE STARS | LOSS RATES | METAL-POOR STARS | O-STARS | GAMMA-RAY BURSTS | VLT-FLAMES SURVEY | galaxies: dwarf | STELLAR EVOLUTION | ASTRONOMY & ASTROPHYSICS | CORE-COLLAPSE SUPERNOVAE | stars: massive | supergiants | ultraviolet: stars | stars: rotation | M-CIRCLE-DOT
Journal Article
Astronomy and astrophysics (Berlin), ISSN 0004-6361, 10/2010, Volume 522, Issue 1, p. A10
Journal Article
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, ISSN 0035-8711, 02/2017, Volume 465, Issue 2, pp. 2294 - 2309
.... In particular, several analyses have demonstrated the possibility to detect non-uniform period spacings, which have been predicted to be directly related to rotation... 
ORDER G-MODES | MODE PERIOD SPACINGS | ANGULAR-MOMENTUM TRANSPORT | stars: interiors | LOW-MASS STARS | MAIN-SEQUENCE STARS | RED GIANTS | TO-CORE ROTATION | KIC 10080943 | asteroseismology | stars: oscillations | A-TYPE STARS | ASTRONOMY & ASTROPHYSICS | KEPLER OBSERVATIONS | stars: rotation | Physics - Solar and Stellar Astrophysics
Journal Article