Astronomical Applications of Astrometry: The Hipparcos and Tycho Catalogues

By M. Perryman. 2008

1,270 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics, Computational Mechanics, Oceanography

View Paper: https://www.semanticscholar.org/paper/67d4d1855a52037d1810798676877f1bd96f1def

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In Astronomy and Astrophysics

1. Michael C. Liu
2. Eric Mamajek
3. K. Luhman
4. A. Burgasser
5. T. Dupuy
6. L. Hillenbrand
7. J. D. Kirkpatrick
8. Kelle Cruz

In Computational Mechanics

1. Eric Mamajek
2. J. D. Kirkpatrick
3. Kelle Cruz
4. I. Neill Reid
5. Santi Cassisi
6. N. Turner
7. Finlay S. Mungall
8. P. Lowrance

In Oceanography

1. Finlay S. Mungall
2. P. Lowrance
3. Eric Mamajek
4. J. D. Kirkpatrick
5. A. Rodr'iguez-Casal
6. Wenceslao González-Manteiga
7. Eduardo Garc'ia-Portugu'es
8. Antonio Cuevas

Citations in the corpus

• DISCOVERY OF A FAINT COMPANION TO ALCOR USING MMT/AO 5 μm IMAGING (2009, background): “Mizar A was also one of the first binary stars to be resolved using an optical interferometer (Pease 1925). The Gliese CNS3 catalog lists the Mizar–Alcor system as a “wide binary and multiple system,” and the 17th widest multiple system in their census of solar neighborhood stars (Gliese & Jahreiß 1”
• Rotational velocities of A-type stars - IV. Evolution of rotational velocities (2012, background): “The shaping of the internal distribution of the stored angular momentum is certainly a matter of hydrodynamical instabilities (Endal & Sofia 1981; Stauffer et al. 1984; Pinsonneault et al. 1990; MacGregor & Brenner 1991; Keppens et al. 1995; Soderblom et al. 1993, 2001), couplings between Full…”
• Rotational velocities of A-type stars. III. Velocity distributions (2006, methodology): “′′15, ESA 1997) or those with large magnitude difference (∆Hp > 3.5–4mag).”
• A SURVEY OF STELLAR FAMILIES: MULTIPLICITY OF SOLAR-TYPE STARS (2009, background): “(2001) with AO at the Mount Wilson Observatory and confirmed by Patience et al. (2002b), who demonstrated CPM and measured infrared magnitudes consistent with the primary’s distance. Four CfA velocity measures over 25 years show a slow downward drift, consistent with this companion. This system also”
• MEETING THE COOL NEIGHBORS. X. ULTRACOOL DWARFS FROM THE 2MASS ALL-SKY DATA RELEASE (2008, methodology): “The overall statistics for activity among ultracool dwarfs are discussed by Schmidt et al. (2007), and we consider the 20-parsec L dwarfs in §5.”
• PLUG‐IN ESTIMATION OF GENERAL LEVEL SETS (2006, methodology): “European Space Agency (1997).”