collaborators

12 papers

astro-ph.GA2026

Angular momentum in isolated disc galaxies: Insights from TNG100

A. Sorgho, L. Verdes-Montenegro, M. Baes +5

Angular momentum is a fundamental property that shapes the evolution of disc galaxies, strongly influencing the internal mechanisms that regulate star formation. Its content within…

astro-ph.GA2026

The size of the HI disk across different environments: isolated, compact groups, clusters, and pairs

R. Ianjamasimanana, L. Verdes-Montenegro, K. M. Hess +8

The 21 cm line of atomic hydrogen (HI) is a sensitive tracer of the outer disk of galaxies, where environmental signatures are most apparent. The relative extent of HI disks compar…

astro-ph.GA2026

Resolved HI and Environmental Dynamics

M. Ramatsoku, P. Serra, N. Deg +8

Spatially resolved, deep HI observations from SKA precursors and pathfinders such as MeerKAT, FAST, and ASKAP have demonstrated their ability to reveal the complex interactions bet…

astro-ph.GA2026

Ram-pressure signatures in the dwarf irregular galaxy SextansB revealed by deep MeerKAT HI observations

Brenda Namumba, Neel Kolhe, Francois Hammer +12

The impact of extremely low-density environments such as the diffuse intergalactic medium (IGM) on the neutral gas distribution of dwarf galaxies remains poorly explored observatio…

astro-ph.GA2026

WALLABY pilot survey: Blinded by the light -- discovery of a fourth member in the ESO 179-013 system

Rayssa Guimarães Silva, Marco Grossi, Denise R. Gonçalves +12

We present new ASKAP/WALLABY HI observations of the nearby dwarf galaxy system ESO 179-013 (Kathryn's Wheel), the nearest known collisional ring galaxy, located 10 Mpc away in the…

astro-ph.GA2026

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…