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Rotation measure synthesis at the 2 m wavelength of the FAN region: unveiling screens and bubbles

Astronomy and astrophysics (Berlin), 2013-01, Vol.549, p.1-16

2013

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The large-scale magnetic field in the fourth Galactic quadrant

Astronomy and astrophysics (Berlin), 2010-04, Vol.513, p.A65

2010

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The ESO Nearby Abell Cluster survey: XIII. The orbits of the different types of galaxies in rich clusters

Astronomy and astrophysics (Berlin), 2004-09, Vol.424 (3), p.779-791

2004

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WSRT Faraday tomography of the Galactic ISM at λ ∼ 0.86 m I. The GEMINI data set at (I, b) = (181°, 20°)

Astronomy and astrophysics (Berlin), 2009-02, Vol.494 (2), p.611-622

2009

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The ESO Nearby Abell Cluster Survey: XI. Segregation of cluster galaxies and subclustering

Astronomy and astrophysics (Berlin), 2002-05, Vol.387 (1), p.8-25

2002

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The ESO nearby Abell cluster survey IX. The morphology-radius and morphology-density relations in rich galaxy clusters

Astronomy and astrophysics (Berlin), 2006-01, Vol.446 (1), p.31-38

2006

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WSRT faraday tomography of the galactic ISM at λ ∼ 0.86 m : First results for a field at (l, b) = (181°, 20°)

Astronomy and astrophysics (Berlin), 2007-08, Vol.471 (2)

2007

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Structure in the polarized Galactic synchrotron emission, in particular “depolarization canals”

Astronomy and astrophysics (Berlin), 2004-11, Vol.427 (2), p.549-559

2004

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On the dynamics of the cores of galaxy clusters

Monthly notices of the Royal Astronomical Society, 1996-03, Vol.279 (2), p.349-388

1996

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The ESO nearby Abell cluster survey VIII. Morphological and spectral classification of galaxies

Astronomy and astrophysics (Berlin), 2006-01, Vol.446 (1), p.19-29

2006

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Characteristics of the structure in the Galactic polarized radio background at 350 MHz

Astronomy and astrophysics (Berlin), 2003-06, Vol.403 (3), p.1045-1057

2003

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Properties of the warm magnetized ISM, as inferred from WSRT polarimetric imaging

Astronomy and astrophysics (Berlin), 2004-11, Vol.427 (1), p.169-177

2004

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The WENSS & Dwingeloo surveys and the Galactic magnetic field

Astronomy and astrophysics (Berlin), 2007-01, Vol.461 (3), p.963-976

2007

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WSRT Faraday tomography of the Galactic ISM at $\mathsf{\lambda \sim 0.86}$ m

Astronomy and astrophysics (Berlin), 2007-08, Vol.471 (2), p.L21-L24

2007

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The ESO Nearby Abell Cluster Survey. XII. The Mass and Mass-to-Light Ratio Profiles of Rich Clusters

The Astrophysical journal, 2004-01, Vol.600 (2), p.657-669

2004

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The ESO Nearby Abell Cluster Survey: V. The catalogue: Contents and instructions for use

Astronomy & astrophysics. Supplement series, 1998-04, Vol.129 (2), p.399-412

1998

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The ESO nearby Abell cluster survey

Astronomy and astrophysics (Berlin), 2006-01, Vol.446 (1), p.19-29

2006

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The ESO nearby Abell cluster survey

Astronomy and astrophysics (Berlin), 2006-01, Vol.446 (1), p.31-38

2006

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The shapes of galaxy clusters

Monthly notices of the Royal Astronomical Society, 1995-03, Vol.273 (1), p.30-46

1995

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A catalogue of galaxy cluster models

Monthly notices of the Royal Astronomical Society, 1997-08, Vol.289 (2), p.327-348

1997

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The ESO Nearby Abell Cluster Survey

Astronomy and astrophysics (Berlin), 2004-09, Vol.424 (3), p.779-791

2004

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WSRT Faraday tomography of the Galactic ISM at λ ~ 0.86 m

Astronomy and astrophysics (Berlin), 2009-02, Vol.494 (2), p.611-622

2009

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WSRT Faraday tomography of the Galactic ISM at \mathsf{\lambda \sim 0.86} m First results for a field at ( l, b) similar to = similar to \mathsf{(181\degr,20\degr) }

Astronomy and astrophysics (Berlin), 2007-01, Vol.471 (2), p.L21-L24

2007

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WSRT Faraday tomography of the Galactic ISM at $\mathsf{\lambda \sim 0.86}$ m: First results for a field at ( l, b )$~=~\mathsf{(181\degr,20\degr)}

Astronomy and astrophysics (Berlin), 2007-08, Vol.471 (2), p.L21-L24

2007

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Radio polarization and RM structure at high Galactic latitudes

Astronomische Nachrichten, 2006-06, Vol.327 (5-6), p.487-490

2006

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Rotation measure synthesis at the 2 m wavelength of the FAN region: unveiling screens and bubbles

The large-scale magnetic field in the fourth Galactic quadrant

The ESO Nearby Abell Cluster survey: XIII. The orbits of the different types of galaxies in rich clusters

WSRT Faraday tomography of the Galactic ISM at λ ∼ 0.86 m I. The GEMINI data set at (I, b) = (181°, 20°)

The ESO Nearby Abell Cluster Survey: XI. Segregation of cluster galaxies and subclustering

The ESO nearby Abell cluster survey IX. The morphology-radius and morphology-density relations in rich galaxy clusters

WSRT faraday tomography of the galactic ISM at λ ∼ 0.86 m : First results for a field at (l, b) = (181°, 20°)

Structure in the polarized Galactic synchrotron emission, in particular “depolarization canals”

On the dynamics of the cores of galaxy clusters

The ESO nearby Abell cluster survey VIII. Morphological and spectral classification of galaxies

Characteristics of the structure in the Galactic polarized radio background at 350 MHz

Properties of the warm magnetized ISM, as inferred from WSRT polarimetric imaging

The WENSS & Dwingeloo surveys and the Galactic magnetic field

WSRT Faraday tomography of the Galactic ISM at $\mathsf{\lambda \sim 0.86}$ m

The ESO Nearby Abell Cluster Survey. XII. The Mass and Mass-to-Light Ratio Profiles of Rich Clusters

The ESO Nearby Abell Cluster Survey: V. The catalogue: Contents and instructions for use

The ESO nearby Abell cluster survey

The ESO nearby Abell cluster survey

The shapes of galaxy clusters

A catalogue of galaxy cluster models

The ESO Nearby Abell Cluster Survey

WSRT Faraday tomography of the Galactic ISM at λ ~ 0.86 m

WSRT Faraday tomography of the Galactic ISM at \mathsf{\lambda \sim 0.86} m First results for a field at ( l, b) similar to = similar to \mathsf{(181\degr,20\degr) }

WSRT Faraday tomography of the Galactic ISM at $\mathsf{\lambda \sim 0.86}$ m: First results for a field at ( l, b )$~=~\mathsf{(181\degr,20\degr)}

Radio polarization and RM structure at high Galactic latitudes

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