activity
20192024
most citedHigh velocity string of knots in the outburst of the Planetary Nebula Hb4

21 citations · 84 across the 10 of their papers we have counts for

collaborators

9 papers

astro-ph.SR2024

Planetary Nebula NGC 2818: Revealing its complex 3D morphology

Sophia Derlopa, Stavros Akras, Philippe Amram +3

We carry out an advanced morpho-kinematic analysis of the Planetary Nebula (PN) NGC 2818, whose complex morphology is described by a basic bipolar component, filamentary structures…

astro-ph.HE2024★ 3 cited

Two shell- and wing-shaped supernova remnants. Investigating the molecular environments around VRO 42.05.01 and G 350.0-2.0

Maria Arias, Ping Zhou, Alexandros Chiotellis +6

Supernova remnants (SNRs) are profoundly affected by their ambient medium. We present carbon monoxide (CO) observations around two mixed morphology SNRs, VRO 42.05.01 and G 350.0-2…

astro-ph.SR2022★ 2 cited

Discovery of an optical cocoon tail behind the runaway HD 185806

Z. T. Spetsieri, P. Boumis, A. Chiotellis +6

Studies on the circumstellar structures around evolved stars provide vital information on the evolution of the parent star and the properties of the local interstellar medium. In t…

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.SR2020★ 13 cited

Two New Nova Shells associated with V4362 Sagittarii and DO Aquilae

E. J. Harvey, M. P. Redman, P. Boumis +8

A classical nova is an eruption on the surface of a white dwarf in an accreting binary system. The material ejected from the white dwarf surface generally forms an axisymmetric she…

astro-ph.HE2020★ 10 cited

First 3D Morpho-Kinematic model of Supernova Remnants. The case of VRO 42.05.01 (G 166.0+4.3)

Sophia Derlopa, Panos Boumis, Alexandros Chiotellis +2

We present the first three dimensional (3D) Morpho-Kinematic (MK) model of a supernova remnant (SNR), using as a case study the Galactic SNR VRO 42.05.01. We employed the astrophys…