Nils H. Turner focuses on Astrophysics, Astronomy, Stars, CHARA array and Interferometry. His work on Spectral energy distribution, Vega and Red giant as part of general Astronomy research is often related to Orbital motion, thus linking different fields of science. His Stars study combines topics from a wide range of disciplines, such as Luminosity and Radius.
Nils H. Turner has included themes like Metallicity and Hertzsprung–Russell diagram in his Radius study. The CHARA array study combines topics in areas such as Telescope, Angular diameter, Astronomical interferometer, Debris disk and Asteroseismology. The Interferometry study which covers Angular resolution that intersects with Remote sensing.
Nils H. Turner mainly focuses on Astrophysics, CHARA array, Astronomy, Stars and Interferometry. His research in Astrophysics tackles topics such as Radius which are related to areas like Asteroseismology. His CHARA array study combines topics in areas such as Gravity darkening, Astronomical interferometer, Effective temperature and Luminosity.
He frequently studies issues relating to Speckle pattern and Astronomy. His biological study spans a wide range of topics, including Angular resolution, Telescope, Remote sensing and Cepheid variable. His Binary star research incorporates themes from Astrometry and Speckle imaging.
His main research concerns Astrophysics, CHARA array, Stars, Interferometry and Astronomy. His Astrophysics research incorporates elements of Radius and Parallax. Nils H. Turner has researched CHARA array in several fields, including Astronomical interferometer, Adaptive optics and Binary star.
The Exoplanet, Starspot and Effective temperature research he does as part of his general Stars study is frequently linked to other disciplines of science, such as Sequence and Orbital motion, therefore creating a link between diverse domains of science. His studies deal with areas such as Cepheid variable, Limb darkening, Photometry, Eclipse and Sigma as well as Interferometry. His work in the fields of Astronomy, such as Brightness, Spectroscopy and Circumstellar disk, intersects with other areas such as Chara and Baseline.
Nils H. Turner focuses on Astrophysics, Stars, Astronomy, Interferometry and CHARA array. His study looks at the relationship between Astrophysics and topics such as Parallax, which overlap with Triple system and Sigma. His work is dedicated to discovering how Stars, Radius are connected with Planetary system, Circumstellar habitable zone, Stellar mass and Spectral energy distribution and other disciplines.
Astronomy is closely attributed to Rotation in his study. Nils H. Turner works mostly in the field of Interferometry, limiting it down to topics relating to Cepheid variable and, in certain cases, Photometry and Infrared excess, as a part of the same area of interest. The study incorporates disciplines such as Navy Precision Optical Interferometer and Washington Double Star Catalog in addition to CHARA array.
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Stellar Diameters and Temperatures II. Main Sequence K & M Stars
Tabetha S. Boyajian;Kaspar von Braun;Gerard van Belle;Harold A. McAlister.
arXiv: Solar and Stellar Astrophysics (2012)
Stellar Diameters and Temperatures. II. Main-sequence K- and M-stars
Tabetha S. Boyajian;Kaspar Von Braun;Gerard Van Belle;Harold A. McAlister.
The Astrophysical Journal (2012)
First Results from the CHARA Array. II. A Description of the Instrument
T. A. ten Brummelaar;H. A. McAlister;S. T. Ridgway;W. G. Bagnuolo.
arXiv: Astrophysics (2005)
First Results from the CHARA Array. II. A Description of the Instrument
T. A. ten Brummelaar;H. A. McAlister;S. T. Ridgway;W. G. Bagnuolo.
The Astrophysical Journal (2005)
Imaging the Surface of Altair
John D. Monnier;M. Zhao;E. Pedretti;N. Thureau.
Science (2007)
Stellar Diameters and Temperatures III. Main Sequence A, F, G, & K Stars: Additional high-precision measurements and empirical relations
Tabetha S. Boyajian;Kaspar von Braun;Gerard van Belle;Chris Farrington.
arXiv: Solar and Stellar Astrophysics (2013)
Stellar Diameters and Temperatures I. Main Sequence A, F, & G Stars
Tabetha S. Boyajian;Harold A. McAlister;Gerard van Belle;Douglas R. Gies.
arXiv: Solar and Stellar Astrophysics (2011)
Fundamental properties of stars using asteroseismology from Kepler and CoRoT and interferometry from the CHARA Array
D. Huber;D. Huber;M. J. Ireland;M. J. Ireland;M. J. Ireland;T. R. Bedding;I. M. Brandão.
The Astrophysical Journal (2012)
First Results from the CHARA Array. VII. Long-Baseline Interferometric Measurements of Vega Consistent with a Pole-On, Rapidly Rotating Star
J. P. Aufdenberg;A. Mérand;V. Coudé du Foresto;Olivier Absil.
The Astrophysical Journal (2006)
STELLAR DIAMETERS AND TEMPERATURES. III. MAIN-SEQUENCE A, F, G, AND K STARS: ADDITIONAL HIGH-PRECISION MEASUREMENTS AND EMPIRICAL RELATIONS
Tabetha S. Boyajian;Tabetha S. Boyajian;Kaspar von Braun;Kaspar von Braun;Gerard van Belle;Chris Farrington.
The Astrophysical Journal (2013)
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