activity
19972017
most citedRadiation driven winds from luminous accretion disks

210 citations · 1.4k across the 24 of their papers we have counts for

collaborators

23 papers

astro-ph.SR2017★ 17 cited

The binary fraction of planetary nebula central stars: the promise of VPHAS+

Helen Barker, Albert Zijlstra, Orsola De Marco +5

The majority of planetary nebulae (PNe) are not spherical, and current single-star models cannot adequately explain all the morphologies we observe. This has led to the Binary Hypo…

astro-ph.SR2017★ 155 cited

VIRAC: The VVV Infrared Astrometric Catalogue

L. C. Smith, P. W. Lucas, R. Kurtev +12

We present VIRAC version 1, a near-infrared proper motion and parallax catalogue of the VISTA VVV survey for 312,587,642 unique sources averaged across all overlapping pawprint and…

astro-ph.SR2014★ 66 cited

First release of the IPHAS Catalogue of New Extended Planetary Nebulae

L. Sabin, Q. A. Parker, R. L. M Corradi +21

We present the first results of our search for new, extended Planetary Nebulae (PNe) based on careful, systematic, visual scrutiny of the imaging data from the INT Photometric H-al…

astro-ph.SR2014★ 177 cited

The Second Data Release of the INT Photometric H-Alpha Survey of the Northern Galactic Plane (IPHAS DR2)

Geert Barentsen, H. J. Farnhill, J. E. Drew +50

The INT/WFC Photometric H-Alpha Survey of the Northern Galactic Plane (IPHAS) is a 1800 square degrees imaging survey covering Galactic latitudes |b| < 5 deg and longitudes l = 30…

astro-ph.SR2014★ 16 cited

Novalike Cataclysmic Variables in the Infrared

D. W. Hoard, Knox S. Long, Steve B. Howell +11

Novalike cataclysmic variables have persistently high mass transfer rates and prominent steady state accretion disks. We present an analysis of infrared observations of twelve nova…

astro-ph.GA2011★ 12 cited

A new Planetary Nebula in the outer reaches of the Galaxy

K. Viironen, A. Mampaso, R. L. M. Corradi +11

A proper determination of the abundance gradient in the Milky Way requires the observation of objects at large galactiocentric distances. With this aim, we are exploring the planet…