43 citations · 210 across the 16 of their papers we have counts for
9 papers · 1 filter
HI rotation curves and mass-size relation for 568 galaxies from the Apertif Wide-area Extragalactic Survey
Konstantin Haubner, Federico Lelli, Enrico Di Teodoro +13
The extended HI rotation curves of galaxies are one of the most powerful tools for studying galaxy evolution and for testing different dark matter and modified gravity models. Howe…
The galactic HI-to-halo mass relation from isolated galaxies to cosmological hydrodynamic simulations
Marie Korsaga, Jonathan Freundlich, Benoit Famaey +15
The relation between HI and dark matter (DM) halo masses provides key insights into gas accretion and the regulation of galaxy formation. In a previous study based on SPARC and LIT…
MeerKAT-64 discovers wide-spread tidal debris in the nearby NGC 7232 galaxy group
Brenda Namumba, Baerbel Silvia Koribalski, Gyula I. G. Józsa +24
We report the discovery of large amounts of previously undetected cold neutral atomic hydrogen (\HI) around the core triplet galaxies in the nearby NGC~7232 galaxy group with MeerK…
A diffuse tidal dwarf galaxy destined to fade out as a "dark galaxy"
Javier Román, Michael G. Jones, Mireia Montes +3
We have explored the properties of a peculiar object detected in deep optical imaging and located at the tip of an HI tail emerging from Hickson Compact Group 16. Using multiband p…
Evolution of compact groups from intermediate to final stages: A case study of the HI content of HCG 16
Michael G. Jones, Lourdes Verdes-Montenegro, Ancor Damas-Segovia +13
Hickson Compact Group (HCG) 16 is a prototypical compact group of galaxies, apparently in an intermediate stage of evolution, where its galaxies are losing gas to the intra-group m…
A Comprehensive Examination of the Optical Morphologies of 719 Isolated Galaxies in the AMIGA Sample
Ronald J. Buta, Lourdes Verdes-Montenegro, Ancor Damas-Segovia +7
Using images from Sloan Digital Sky Survey Data Release 8, we have re-examined the morphology of 719 galaxies from the Analysis of the interstellar Medium in Isolated GAlaxies (AMI…
Unveiling the environment and faint features of the isolated galaxy CIG 96 with deep optical and HI observations
P. Ramirez-Moreta, L. Verdes-Montenegro, J. Blasco-Herrera +21
Asymmetries in HI in galaxies are often caused by the interaction with close companions, making isolated galaxies an ideal framework to study secular evolution. The AMIGA project h…
The AMIGA sample of isolated galaxies XIII. The HI content of an almost "nurture free" sample
Michael G. Jones, Daniel Espada, Lourdes Verdes-Montenegro +8
We present the largest catalogue of HI single dish observations of isolated galaxies to date and the corresponding HI scaling relations, as part of the multi-wavelength project AMI…
Are (pseudo)bulges in isolated galaxies actually primordial relics?
M. Fernández Lorenzo, J. Sulentic, L. Verdes-Montenegro +7
We present structural parameters and (g-i) bulge/disk colors for a large sample (189) of isolated AMIGA galaxies. The structural parameters of bulges were derived from the 2D bulge…