activity
19962025
most citedStochastic modeling of multiwavelength variability of the classical BL Lac object OJ 287 on timescales ranging from decades to hours

81 citations · 791 across the 39 of their papers we have counts for

collaborators

39 papers

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…

astro-ph.SR2024★ 3 cited

Detection of the [C I] 8727 emission line. Low-ionization structures in NGC 7009

Stavros Akras, Hektor Monteiro, Jeremy R. Walsh +5

We report the first spatially resolved detection of the near-infrared [C I] 8727 emission from the outer pair of low-ionization structures in the planetary nebula NGC 7009 from…

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.EP2023★ 10 cited

The Hubble/STIS Near-ultraviolet Transmission Spectrum of HD 189733b

Patricio E. Cubillos, Luca Fossati, Tommi Koskinen +5

The benchmark hot Jupiter HD 189733b has been a key target to lay out the foundations of comparative planetology for giant exoplanets. As such, HD 189733b has been extensively stud…

astro-ph.SR2023

The messy death of a multiple star system and the resulting planetary nebula as observed by JWST

Orsola De Marco, Muhammad Akashi, Stavros Akras +66

Planetary nebulae (PNe), the ejected envelopes of red giant stars, provide us with a history of the last, mass-losing phases of 90 percent of stars initially more massive than the…