activity
20072020
most citedVISTA Variables in the Via Lactea (VVV): The public ESO near-IR variability survey of the Milky Way

1k citations · 3.1k across the 34 of their papers we have counts for

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Showing 2009Show all

6 papers · 1 filter

astro-ph.GA2009★ 1k cited

VISTA Variables in the Via Lactea (VVV): The public ESO near-IR variability survey of the Milky Way

D. Minniti, P. W. Lucas, J. P. Emerson +63

We describe the public ESO near-IR variability survey (VVV) scanning the Milky Way bulge and an adjacent section of the mid-plane where star formation activity is high. The survey…

astro-ph.GA2009★ 59 cited

IPHAS and the symbiotic stars. II. New discoveries and a sample of the most common mimics

R. L. M. Corradi, M. Valentini, U. Munari +19

In a previous paper [arXiv:0712.2391], we presented the selection criteria needed to search for symbiotic stars in IPHAS, the INT Halpha survey of the Northern Galactic plane. IPHA…

astro-ph.GA2009★ 47 cited

The Structure of the Outer Galactic Disc as revealed by IPHAS early A Stars

S. E. Sale, J. E. Drew, C. Knigge +10

This study is an investigation of the stellar density profile of the Galactic disc in the Anticentre direction. We select over 40,000 early A stars from IPHAS photometry in the Gal…

astro-ph.GA2009★ 56 cited

The UV-Excess Survey of the Northern Galactic Plane (UVEX)

Paul J. Groot, K. Verbeek, R. Greimel +41

The UV-Excess Survey of the Northern Galactic Plane images a 10x185 degree wide band, centered on the Galactic Equator using the 2.5m Isaac Newton Telescope in four bands (U,g,r,He…

astro-ph.GA2009★ 35 cited

New Young Planetary Nebulae in IPHAS

K. Viironen, A. Mampaso, R. L. M. Corradi +12

We search for very small-diameter galactic planetary nebulae (PNe) representing the earliest phases of PN evolution. A recently published IPHAS catalogue of Ha-emitting stars provi…

astro-ph.SR2009★ 6 cited

Central Stars of Planetary Nebulae in IPHAS and SDSS

S. Weston, R. Napiwotzki, S. Sale

Space densities and birthrates of Planetary Nebulae (PNe) are highly uncertain. A large range of formation rates has been derived by different studies, which has led to contradicti…