Post-AGB stars
H Van Winckel - Annual Review of Astronomy and Astrophysics, 2003 - annualreviews.org
▪ Abstract In this contribution, a review is presented on the ample data obtained on post-AGB
stars, both on the central stars and their circumstellar material. The fast evolutionary phase is …
stars, both on the central stars and their circumstellar material. The fast evolutionary phase is …
Carbon stars
G Wallerstein, GR Knapp - Annual Review of Astronomy and …, 1998 - annualreviews.org
▪ Abstract Absolute magnitudes are estimated for carbon stars of various subtypes in the
Hipparcos catalogue and as found in the Magellanic Clouds. Stellar radii fall within the limits …
Hipparcos catalogue and as found in the Magellanic Clouds. Stellar radii fall within the limits …
Dephasing in electron interference by a 'which-path'detector
Wave–particle duality, as manifest in the two-slit experiment, provides perhaps the most
vivid illustration of Bohr's complementarity principle: wave-like behaviour (interference) …
vivid illustration of Bohr's complementarity principle: wave-like behaviour (interference) …
Bipolar pre-planetary nebulae: hydrodynamics of dusty winds in binary systems. II. Morphology of the circumstellar envelopes
N Mastrodemos, M Morris - The Astrophysical Journal, 1999 - iopscience.iop.org
We have constructed three-dimensional smoothed particle hydrodynamics models to
examine the influence of a detached binary companion on the dusty winds from red giants …
examine the influence of a detached binary companion on the dusty winds from red giants …
Keplerian discs around post-AGB stars: a common phenomenon?
S De Ruyter, H Van Winckel, T Maas, TL Evans… - Astronomy & …, 2006 - aanda.org
Aims. We aim at showing that the broad-band SED characteristics of our sample of post-AGB
stars are best interpreted, assuming the circumstellar dust is stored in Keplerian rotating …
stars are best interpreted, assuming the circumstellar dust is stored in Keplerian rotating …
An oxygen-rich dust disk surrounding an evolved star in the Red Rectangle
L Waters, C Waelkens, H Van Winckel, FJ Molster… - Nature, 1998 - nature.com
Abstract The Red Rectangle is the prototype of a class of carbon-rich reflection nebulae
surrounding low-mass stars in the final stages of evolution. The central star of this nebula …
surrounding low-mass stars in the final stages of evolution. The central star of this nebula …
The formation of very narrow waist bipolar planetary nebulae
N Soker, S Rappaport - The Astrophysical Journal, 2000 - iopscience.iop.org
We discuss the interaction of the slow wind blown by an asymptotic giant branch (AGB) star
with a collimated fast wind (CFW) blown by its main-sequence or white dwarf companion, at …
with a collimated fast wind (CFW) blown by its main-sequence or white dwarf companion, at …
Crystalline silicate dust around evolved stars-I. The sample stars
This is the first paper in a series of three where we present the first comprehensive inventory
of solid state emission bands observed in a sample of 17 oxygen-rich circumstellar dust …
of solid state emission bands observed in a sample of 17 oxygen-rich circumstellar dust …
Hubble Space Telescope imaging of HD 44179, the red rectangle
M Cohen, H Van Winckel, HE Bond… - The Astronomical …, 2004 - iopscience.iop.org
Abstract We present Hubble Space Telescope (HST) Wide Field Planetary Camera 2 and
deep ground-based images of the Red Rectangle (RR), a bipolar proto–planetary nebula …
deep ground-based images of the Red Rectangle (RR), a bipolar proto–planetary nebula …
Discovery of far-infrared pure rotational transitions of CH+ in NGC 7027
J Cernicharo, XW Liu, E González-Alfonso… - The Astrophysical …, 1997 - iopscience.iop.org
We report the discovery of the rotational spectrum of CH+ in the Infrared Space Observatory
Long Wavelength Spectrometer (LWS) spectrum of the planetary nebula NGC 7027. The …
Long Wavelength Spectrometer (LWS) spectrum of the planetary nebula NGC 7027. The …