activity
19992007
most citedA Grand Challenge for Planetary Nebulae

5 citations · 9 across the 5 of their papers we have counts for

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astro-ph20075 cited

A Grand Challenge for Planetary Nebulae

Adam Frank, Orsola De Marco, Eric Blackman +1

The study of PN has been confronting a growing list of dilemmas which have yet to find coherent resolution. These issues are both observational and theoretical and can be stated as…

astro-ph20071 cited

[WC] and PG1159 Central Stars of Planetary Nebula: the Need for an Alternative to the Born-Again Scenario

Orsola De Marco

Hydrogen-deficient central stars of planetary nebula such as Wolf-Rayet and PG1159 central stars and some weak emission line stars are primarily composed of helium and carbon. This…

astro-ph20071 cited

The Bizarre Spectral Variability of Central Stars of Planetary Nebulae

Orsola De Marco, S. Wortel, Howard E. Bond +1

A radial velocity (RV) survey to detect central stars in binary systems was carried out between 2002 and 2004. De Marco et al. (2004) reported that 10 out of 11 monitored stars exh…

astro-ph2003

Outflows and Jets I: a personal take

Orsola De Marco

As a session chair I have the privilege to write down a few comments on four talks that were delivered under the general title of "outflows and jets I". This and the session that f…

astro-ph20032 cited

The dual dust chemistry - binarity connection

Orsola De Marco, A. F. Jones, M. J. Barlow +1

Accumulating evidence points to a binary nature for the Wolf-Rayet ([WC]) central stars, a group that constitutes about 15% of all central stars of planetary nebula. From ISO obser…

astro-ph2000

Far-UV FUSE spectroscopy of the OVI resonance doublet in Sand2 (WO)

Paul A. Crowther, A. W. Fullerton, D. J. Hillier +10

We present Far-Ultraviolet Spectroscopic Explorer (FUSE) spectroscopy of Sand 2, a LMC WO-type Wolf-Rayet star, revealing the OVI resonance P Cygni doublet at 1032-38A. These data…