SIMULATING THE COMMON ENVELOPE PHASE OF A RED GIANT USING SMOOTHED-PARTICLE HYDRODYNAMICS AND UNIFORM-GRID CODES
- 13 December 2011
- journal article
- Published by American Astronomical Society in The Astrophysical Journal
- Vol. 744 (1)
- https://doi.org/10.1088/0004-637x/744/1/52
Abstract
No abstract availableOther Versions
This publication has 40 references indexed in Scilit:
- On the α formalism for the common envelope interactionMonthly Notices of the Royal Astronomical Society, 2011
- Compact Object Modeling with the StarTrack Population Synthesis CodeThe Astrophysical Journal Supplement Series, 2008
- Fundamental differences between SPH and grid methodsMonthly Notices of the Royal Astronomical Society, 2007
- Adaptive binning of X-ray data with weighted Voronoi tessellationsMonthly Notices of the Royal Astronomical Society, 2006
- A catalog of rotational and radial velocities for evolved starsAstronomy and Astrophysics Supplement Series, 1999
- The Santa Barbara Cluster Comparison Project: A Comparison of Cosmological Hydrodynamics SolutionsThe Astrophysical Journal, 1999
- A piecewise parabolic method for cosmological hydrodynamicsComputer Physics Communications, 1995
- The effect of an external disk on the orbital elements of a central binaryThe Astrophysical Journal, 1991
- Double-core evolution. II - Two-dimensional hydrodynamic effectsThe Astrophysical Journal, 1984
- On the Mechanism of Accretion by StarsMonthly Notices of the Royal Astronomical Society, 1944