An Introduction to Close Binary Stars: Contents

By R. Hilditch. 2001

216 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics

View Paper: https://www.semanticscholar.org/paper/bf296c6b99f35e1aac6032787b0052714621d360

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In Astronomy and Astrophysics

1. J. Southworth
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Citations in the corpus

• The Rossiter-McLaughlin effect of CoRoT-3b and HD 189733b (2009, methodology): “The RV curve is modelled by the standard orbital equations (Mayor & Queloz 1995; Hilditch 2001) and by the code presented in Giménez (2006b) for the RM effect.”
• KEPLER-413B: A SLIGHTLY MISALIGNED, NEPTUNE-SIZE TRANSITING CIRCUMBINARY PLANET (2014, background): “The former depend on the binary parameters only and can be calculated from Hilditch (2001)4: xs = rs cos(θbin +ωbin) ys = rs sin(θbin +ωbin)cos ibin (4) where rs,ωbin,θbin and ibin can be directly estimated from the radial velocity measurements and from the Kepler light curve.”
• Unique sextuple system: 65 Ursae Majoris (2012, methodology): “Using our new computed parallax and the Kepler’s third law, we calculated the total mass of the system (e.g. Hilditch 2001).”
• Understanding the Lomb–Scargle Periodogram (2017, background): “…1982; Horne & Baliunas 1986; Press et al. 2007), the harmonic mean of the sampling intervals (e.g. Debosscher et al. 2007), the median of the sampling intervals (e.g. Graham et al. 2013b), or the minimum sample spacing (e.g. Percy 1986; Roberts et al. 1987; Press & Rybicki 1989; Hilditch 2001).”
• The Evolutionary Status of Be Stars: Results from a Photometric Study of Southern Open Clusters (2005, background): “Commonly, the mass ratio becomes inverted during the mass transfer and the orbital separation a increases, leading to a dramatic increase in the timescale for tidal synchronization (∼ a17/2; Hilditch 2001).”
• Homogeneous studies of transiting extrasolar planets – IV. Thirty systems with space-based light curves (2011, methodology): “A starting value is guessed, and is combined with the measuredPorb, rA, rb, i andKA to obtain the physical properties of the system using standard formulae (e.g. Hilditch 2001).”
• Eclipsing binaries in open clusters. II. V453 Cyg in NGC 6871 (2004, background): “The time-scale for orbital circularization is about 1.5 Gyr (Zahn 1977; Hilditch 2001) which is consistent with the presence of a small but well-defined eccentricity.”
• Homogeneous studies of transiting extrasolar planets - III. Additional planets and stellar models (2010, methodology): “The uncertainty in Porb is generally negligible, andT0 does not enter theABSDIM analysis. c© 0000 RAS, MNRAS000, 000–000 is defined, usually in the region of 150 km s−1, and the full physical properties of the system are calculated using standard formulae (e.g. Hilditch 2001).”