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papers

Publications (23)

Secular Evolution of Galaxy Morphologies

D. Pfenniger, L. Martinet, F. Combes

First Results from ISOCAM Images of Circumnuclear Starbursts in Barred Galaxies

H. Wozniak, D. Friedli, L. Martinet +1

Is Dark Matter in Spiral Galaxies Cold Gas? II. Fractal Models and Star Non-Formation

D. Pfenniger, F. Combes

Perspectives for detecting cold H2 in outer galactic disks

F. Combes, D. Pfenniger

Molecular gas in high-velocity clouds: revisited scenario

M. Dessauges-Zavadsky, F. Combes, D. Pfenniger

Fractal Cold Gas as Dark Matter in Galaxies and Clusters

D. Pfenniger, F. Combes

Formation of massive counter-rotating disks: an alternative scenario

I. Puerari, D. Pfenniger

Stellar Dynamics and the 3D Structure of Bars

D. Pfenniger

Possible flakes of molecular hydrogen in the early Universe

D. Pfenniger, D. Puy

astro-ph.GA2009

Simulations of galactic disks including an additional dark baryonic component

Y. Revaz, D. Pfenniger, F. Combes +1

Bending instabilities at the origin of persistent warps

Y. Revaz, D. Pfenniger

The Baryonic Tully-Fisher relation revisited

D. Pfenniger, Y. Revaz

Periodic orbits in warped disk

Y. Revaz, D. Pfenniger

astro-ph.GA2014

CO map and steep Kennicutt-Schmidt relation in the extended UV disk of M63

M. Dessauges-Zavadsky, C. Verdugo, F. Combes +1

Making Spirals with Counter-Rotating Disks, the case of NGC 4550

D. Pfenniger

News on Dark Matter in Galaxies and Clusters

F. Combes, D. Pfenniger

Very Cold Gas and Dark Matter

F. Combes, D. Pfenniger

Simulations of galactic disks including a dark baryonic component

Y. Revaz, D. Pfenniger, F. Combes +1

Is Dark Matter in Spiral Galaxies Cold Gas? I. Observational Constraints and Dynamical Clues About Galaxy Evolution

D. Pfenniger, F. Combes, L. Martinet

Clumpuscule Formation at High Redshift

F. Combes, D. Pfenniger

Fundamental Aspects of the ISM Fractality

D. Pfenniger

astro-ph.CO2013

On the detection of point sources in CMB maps

H. G. Khachatryan, G. Nurbaeva, D. Pfenniger +1

ISOCAM images at 6.75 and 15 microns: the circumnuclear region of NGC 4321 (M 100)

H. Wozniak, D. Friedli, L. Martinet +1