activity
20242026
collaborators

9 papers

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

J-PLUS: The planetary nebula population of M 33

Giovanna Liberato, Denise R. Gonçalves, Arianna Cortesi +21

In this pilot study, we investigate the PN population in M~33, a nearby spiral galaxy (~kpc), using data from the DR3 of the Javalambre-Photometric Local Universe Surve…

astro-ph.SR2025

PHR~J1724-3859: A Bipolar Planetary Nebula in Open Cluster Trumpler 25

Vasiliki Fragkou, Quentin A. Parker, Denise R. Gonçalves

Planetary nebulae (PNe) studies are essential for understanding late stellar evolution of low-to-intermediate mass stars. PNe in open clusters (OC) are rare but valuable since thei…

astro-ph.GA2025

Low-ionization structures in planetary nebulae -- IV. The molecular hydrogen counterpart

M. B. Mari, S. Akras, D. R. Gonçalves

Context. Low-ionization structures (LISs), found in all morphological types of planetary nebulae (PNe), are small-scale features prominent in emission from low-ionization species s…

astro-ph.GA2025

The Local Group Symbiotic Star Population and its Tenuous Link with Type Ia Supernovae

Marco Laversveiler, Denise R. Gonçalves, Helio J. Rocha-Pinto +1

Binary stars are gravitationally bound stellar systems where the evolution of each component can significantly influence the evolution of its companion and the system as a whole. I…

astro-ph.SR2025

Integral field spectroscopy of the planetary nebula NGC 3242 and the puzzling nature of its low ionization structures

L. Konstantinou, S. Akras, J. Garcia-Rojas +7

The physico-chemical properties of the planetary nebula (PN) NGC 3242 are investigated in both 1D and 2D, using Integral Field Unit (IFU) data. This PN has a complex morphology wit…