activity
20042007
most citedDiscovery of photospheric argon in very hot central stars of planetary nebulae and white dwarfs

43 citations · 157 across the 5 of their papers we have counts for

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7 papers · 1 filter

astro-ph2007

3D Photoionisation Modelling of NGC 6302

N. J. Wright, M. J. Barlow, B. Ercolano +1

We present a three-dimensional photoionisation and dust radiative transfer model of NGC 6302, an extreme, high-excitation planetary nebula. We use the 3D photoionisation code Mocas…

astro-ph200731 cited

Identification of NeVIII lines in H-deficient (pre-) white dwarfs: a new tool to constrain the temperature of the hottest stars

K. Werner, T. Rauch, J. W. Kruk

For the first time, we have identified NeVIII absorption lines in far-UV spectra of the hottest known (Teff>150,000 K) hydrogen-deficient (pre-) white dwarfs of spectral type PG115…

astro-ph200743 cited

Discovery of photospheric argon in very hot central stars of planetary nebulae and white dwarfs

K. Werner, T. Rauch, J. W. Kruk

We report the first discovery of argon in hot evolved stars and white dwarfs. We have identified the ArVII 1063.55A line in some of the hottest known (Teff=95000-110000 K) central…

astro-ph200641 cited

High-resolution ultraviolet spectroscopy of PG1159-035 with HST and FUSE

D. Jahn, T. Rauch, E. Reiff +3

PG1159-035 is the prototype of the PG1159 spectral class which consists of extremely hot hydrogen-deficient (pre-) white dwarfs. It is also the prototype of the GW Vir variables, w…

astro-ph200642 cited

VLT spectroscopy and non-LTE modeling of the C/O-dominated accretion disks in two ultracompact X-ray binaries

K. Werner, T. Nagel, T. Rauch +2

We present new medium-resolution high-S/N optical spectra of the ultracompact low-mass X-ray binaries 4U0614+091 and 4U1626-67, taken with the ESO Very Large Telescope. They are pu…

astro-ph2004

Identification of neon in FUSE and VLT spectra of extremely hot hydrogen-deficient (pre-) white dwarfs

K. Werner, T. Rauch, E. Reiff +2

One of the strongest absorption lines observed in far-ultraviolet FUSE spectra of many PG1159 stars remained unidentified up to now. We show that this line, located at 973.3A, stem…