activity
20162026
most citedThe Planetary Nebula in the 500 Myr old Open Cluster M37

21 citations · 89 across the 12 of their papers we have counts for

collaborators

12 papers

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★ 2 cited

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.SR2025

Near-infrared photometry of the central stars of planetary nebulae with the VVVX survey

Dante Minniti, Vasiliki Fragkou, Javier Alonso-García +2

Achieving accurate photometric characterizations of central stars of planetary nebulae (CSPNe) toward the galactic plane is significantly hindered by the high levels of interstella…

astro-ph.SR2025★ 7 cited

The physical association of planetary nebula NGC 2818 with open cluster NGC 2818A

Vasiliki Fragkou, Roberto Vázquez, Quentin A. Parker +2

Planetary nebulae (PNe) that are physical members of open star clusters (OCs) are valuable for stellar evolution studies. They are extremely rare, with only three such instances co…

astro-ph.GA2025

The S-PLUS Fornax Project (S+FP): Mapping globular clusters systems within 5 virial radii around NGC 1399

Luis Lomelí-Núñez, A. Cortesi, A. V. Smith Castelli +25

We present the largest sample (13,000 candidates, 3000 of wich are bona-fide candidates) of globular cluster (GCs) candidates reported in the Fornax Cluster so far. The…

astro-ph.SR2022★ 21 cited

The Planetary Nebula in the 500 Myr old Open Cluster M37

Vasiliki Fragkou, Quentin A. Parker, Albert A. Zijlstra +3

We report confirmation of a large, evolved, bipolar planetary nebula and its blue, white dwarf central star as a member of the ~500 Myr old Galactic open star cluster M37 (NGC 2099…

astro-ph.GA2022★ 15 cited

Deep optical study of the mixed-morphology supernova remnant G 132.7+1.3 (HB3)

P. Boumis, A. Chiotellis, V. Fragkou +8

We present optical ccd images of the large supernova remnant (SNR) G132.71.3 (HB3) covering its full extent for the first time, in the emission lines of H[N II], [S II] and…

astro-ph.SR2019★ 16 cited

A high-mass Planetary Nebula in a Galactic Open Cluster

Vasiliki Fragkou, Quentin Parker, Albert Zijlstra +2

Planetary Nebulae are the ionised ejected envelopes surrounding the remnant cores of dying stars. Theory predicts that main-sequence stars with one to about eight times the mass of…

astro-ph.SR2019★ 10 cited

The Central Star of Planetary Nebula PHR 1315-6555 and its host Galactic Open Cluster AL 1

V. Fragkou, Q. A. Parker, A. A. Zijlstra +2

PHR 1315-6555 is a rare case of a Galactic Planetary Nebula that is a proven member of the Open Cluster AL 1. This allows its distance to be defined with precision and thus the acc…

astro-ph.SR2018

Central Stars of Planetary Nebulae in Galactic Open Clusters: Providing additional data for the White Dwarf Initial-to-Final-Mass Relation

Vasiliki Fragkou, Quentin A. Parker, Albert Zijlstra +2

Accurate (<10%) distances of Galactic star clusters allow precise estimation of the physical parameters of any physically associated Planetary Nebula (PN) and also that of its cent…

astro-ph.GA2018★ 15 cited

New Galactic Planetary Nebulae selected by radio and multi-wavelength characteristics

Vasiliki Fragkou, Quentin A. Parker, Ivan S. Bojicic +1

We have used the Cornish radio catalogue combined with the use of multi-wavelength data to identify 62 new Planetary Nebula (PN) candidates close to the Galactic mid-plane. Of this…

astro-ph.GA2016★ 3 cited

Planetary Nebula Candidates Uncovered with the HASH Research Platform

Vasiliki Fragkou, Ivan Bojičić, David Frew +1

A detailed examination of new high quality radio catalogues (e.g. Cornish) in combination with available mid-infrared (MIR) satellite imagery (e.g. Glimpse) has allowed us to find…