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19932008
most citedMagnetic fields in planetary nebulae and post-AGB nebulae

65 citations · 150 across the 9 of their papers we have counts for

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Showing 2007Show all

16 papers · 1 filter

astro-ph200798 cited

Initial Data Release from the INT Photometric H-alpha Survey of the Northern Galactic Plane (IPHAS)

E. A. Gonzalez-Solares, N. A. Walton, R. Greimel +47

The INT/WFC Photometric H-alpha Survey of the Northern Galactic Plane (IPHAS) is an imaging survey being carried out in H-alpha, r' and i' filters, with the Wide Field Camera (WFC)…

astro-ph200731 cited

Dust mass-loss rates from AGB stars in the Fornax and Sagittarius dwarf Spheroidal galaxies

Eric Lagadec, Albert A. Zijlstra, Mikako Matsuura +3

To study the effect of metallicity on the mass-loss rate of asymptotic giant branch (AGB) stars, we have conducted mid-infrared photometric measurements of such stars in the Sagitt…

astro-ph200749 cited

It's a wonderful tail: the mass loss history of Mira

C. J. Wareing, A. A. Zijlstra, T. J. O'Brien +1

Recent observations of the Mira AB binary system have revealed a surrounding arc-like structure and a stream of material stretching 2 degrees away in opposition to the arc. The ali…

astro-ph200738 cited

A disc in the heart of the Ant nebula

Foteini Lykou, Olivier Chesneau, Eric Lagadec +1

We present the discovery of a silicate disc at the centre of the planetary nebula Mz3 (the Ant). The nebula was observed with MIDI on the Very Large Telescope Interferometer (VLTI)…

astro-ph200738 cited

A silicate disk in the heart of the Ant

Olivier Chesneau, Foteini Lykou, Bruce Balick +6

We aim at getting high spatial resolution information on the dusty core of bipolar planetary nebulae to directly constrain the shaping process. Methods: We present observations of…

astro-ph200736 cited

The enigma of the oldest `nova': the central star and nebula of CK Vul

M. Hajduk, Albert A. Zijlstra, P. A. M. van Hoof +9

CK Vul is classified as, amongst others, the slowest known nova, a hibernating nova, or a very late thermal pulse object. Following its eruption in AD 1670, the star remained visib…