Stellar wind models of central stars of planetary nebulae
- 1 March 2020
- journal article
- research article
- Published by EDP Sciences in Astronomy & Astrophysics
- Vol. 635, A173
- https://doi.org/10.1051/0004-6361/201937150
Abstract
Astronomy & Astrophysics (A&A) is an international journal which publishes papers on all aspects of astronomy and astrophysicsKeywords
This publication has 125 references indexed in Scilit:
- MODULES FOR EXPERIMENTS IN STELLAR ASTROPHYSICS (MESA): PLANETS, OSCILLATIONS, ROTATION, AND MASSIVE STARSThe Astrophysical Journal Supplement Series, 2013
- Three-dimensional radiative transfer in clumped hot star windsAstronomy & Astrophysics, 2012
- The cool magnetic DAZ white dwarf NLTT 10480Astronomy & Astrophysics, 2011
- Comoving frame models of hot star windsAstronomy & Astrophysics, 2010
- A GRAVITATIONAL REDSHIFT DETERMINATION OF THE MEAN MASS OF WHITE DWARFS. DA STARSThe Astrophysical Journal, 2010
- Mass loss from inhomogeneous hot star windsAstronomy & Astrophysics, 2010
- Elemental abundances of Galactic bulge planetary nebulae from optical recombination linesMonthly Notices of the Royal Astronomical Society, 2007
- X-ray line emission from a fragmented stellar windAstronomy & Astrophysics, 2003
- Terminal Velocities and the Bistability of Stellar WindsThe Astrophysical Journal, 1995
- Neon-22 as a neutron source, light elements as modulators, and s-process nucleosynthesis in a thermally pulsing starThe Astrophysical Journal, 1975