We infer the central mass distributions within 0.4-1.2 disc scalelengths of 18 late-type spiral galaxies using two different dynamical modelling approaches -...
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PublicationThe inner mass distribution of late-type spiral galaxies from <monospace>SAURON</monospace> stellar kinematic maps
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PublicationThe innermost globular clusters of M87
We present a comprehensive multiwavelength photometric analysis of the innermost (˜3 × 3 kpc2) 110 globular clusters (GCs) of M87. Their spectral energy...
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PublicationThe INT Photometric Hα Survey of the Northern Galactic Plane (IPHAS)
The Isaac Newton Telescope (INT) Photometric Hα Survey of the Northern Galactic Plane (IPHAS) is a 1800-deg2 CCD survey of the northern Milky Way spanning the...
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PublicationThe interaction of the halo around the butterfly planetary nebula NGC 650-1 with the interstellar medium
With its bright and wide equatorial waist seen almost edge-on (`the butterfly body') and the faint and broad bipolar extensions (`the butterfly wings'), NGC 650...
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PublicationThe intermediate polar cataclysmic variable GK Persei 120 years after the nova explosion: a first dynamical mass study
We present a dynamical study of the intermediate polar and dwarf nova cataclysmic variable GK Persei (Nova Persei 1901) based on a multisite optical...
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PublicationThe interstellar medium in the Upper Cepheus-Cassiopeia region
We have studied the kinematics and spatial distribution of the interstellar gas in the sky region 110°
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PublicationThe intracluster light as a tracer of the total matter density distribution: a view from simulations
By using deep observations of clusters of galaxies, it has been recently found that the projected stellar mass density closely follows the projected total (dark...
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PublicationThe intriguing H I gas in NGC 5253: an infall of a diffuse, low-metallicity H I cloud?
We present new, deep H I line and 20-cm radio-continuum data of the very puzzling blue compact dwarf galaxy NGC 5253, obtained with the Australia Telescope...
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PublicationThe intrinsic alignment of red galaxies in DES Y1 redMaPPer galaxy clusters
Clusters of galaxies trace the most non-linear peaks in the cosmic density field. The weak gravitational lensing of background galaxies by clusters can allow us...