173 citations · 1.2k across the 39 of their papers we have counts for
40 papers
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…
IllustrisTNG50 angular momentum maps: tracing the morpho-kinematic evolution of galaxies
Juan Manuel Pacheco-Arias, Benoît Epinat, Philippe Amram +2
Following the first observational study of the two-dimensional spatial distribution of stellar specific angular momentum (sAM) in late-type galaxies, we quantify the morpho-kinemat…
Physical characterization of the local system NGC 1313: A flattening in its chemical abundance by past interactions
Belén Ojeda-Díaz, Sergio Torres-Flores, Daniela E. Olave-Rojas +5
Interacting galaxies provide unique information on morphological transformation, enhanced star formation, and chemical evolution, and thus contribute to understanding the complex e…
New morpho-kinematic classification: The two-dimensional spatial distribution of stellar specific angular momentum in late-type galaxies
Juan Manuel Pacheco-Arias, Philippe Amram, Benoît Epinat +1
The two-dimensional spatial distribution of stellar specific angular momentum (sAM) within galaxies has never been previously analysed. We investigate its morpho-kinematics and its…
WLM: Dynamics of an isolated Dwarf Irregular Galaxy Under Ram Pressure in the Local Group
Neel Kolhe, Francois Hammer, Yanbin Yang +5
WLM is an archetypal dwarf irregular galaxy that has not experienced interactions with major Local Group galaxies within the past 8 Gyr. It has recently been shown that WLM is losi…
Extraplanar emission in isolated edge-on late-type galaxies.II. The H kinematics
Minerva M. Sardaneta, Philippe Amram, Roberto Rampazzo +3
Isolated galaxies are rare yet invaluable for studying secular evolution, as their physical properties can remain largely unaffected by external influences for several billion year…