Search Results - "Chiotellis, A."
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‘Ears’ formation in supernova remnants: overhearing an interaction history with bipolar circumstellar structures
Published in Monthly notices of the Royal Astronomical Society (01-03-2021)“…ABSTRACT A characteristic feature that is frequently found in nearby supernova remnants (SNRs) is the existence of two antisymmetric, local protrusions that…”
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Planetary nebulae hosting accreting white dwarfs: a possible solution for the mysterious cut-off of planetary nebula luminosity function?
Published in Monthly notices of the Royal Astronomical Society (01-05-2023)“…ABSTRACT Many binary companions to the central stars of planetary nebulae (PNe) are found to be inflated, perhaps indicating that accretion onto the central…”
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Planetary Nebula NGC 2818: Revealing its complex 3D morphology
Published in Monthly notices of the Royal Astronomical Society (25-04-2024)“…ABSTRACT We carry out an advanced morpho-kinematic analysis of the Planetary Nebula (PN) NGC 2818, whose complex morphology is described by a basic bipolar…”
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First 3D morpho-kinematic model of supernova remnants. The case of VRO 42.05.01 (G166.0+4.3)
Published in Monthly notices of the Royal Astronomical Society (01-12-2020)“…ABSTRACT 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…”
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The sculpting of rectangular and jet-like morphologies in supernova remnants by anisotropic equatorially confined progenitor stellar winds
Published in Monthly notices of the Royal Astronomical Society (01-03-2023)“…ABSTRACT Thermonuclear and core-collapse supernova remnants (SNRs) are the nebular leftovers of defunct stars. Their morphology and emission properties provide…”
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Modelling the cometary structure of the planetary nebula HFG1 based on the evolution of its binary central star V664 Cas
Published in Monthly notices of the Royal Astronomical Society (21-03-2016)“…HFG1 is the first well-observed planetary nebula (PN) which reveals a cometary-like structure. Its main morphological features consist of a bow-shaped shell,…”
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Detection of optical emission from the supernova remnant G7.7–3.7
Published in Monthly notices of the Royal Astronomical Society (21-09-2023)“…ABSTRACT We present the first optical study of the supernova remnant (SNR) G7.7–3.7, with the aim of determining its evolutionary phase since it has been…”
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Deep optical study of the mixed-morphology supernova remnant G 132.7+1.3 (HB3)
Published in Monthly notices of the Royal Astronomical Society (23-03-2022)“…ABSTRACT We present optical CCD images of the large supernova remnant (SNR) G 132.7+1.3 (HB3) covering its full extent for the first time, in the emission…”
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Linking the properties of accreting white dwarfs with the ionization state of their ambient medium
Published in Monthly notices of the Royal Astronomical Society (05-05-2022)“…ABSTRACT Steadily accreting white dwarfs (WDs) are efficient sources of ionization and thus are able to create extended ionized nebulae in their vicinity…”
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The Interaction of Type Ia Supernovae with Planetary Nebulae: The Case of Kepler’s Supernova Remnant
Published in Galaxies (01-06-2020)“…One of the key methods for determining the unknown nature of Type Ia supernovae (SNe Ia) is the search for traces of interaction between the SN ejecta and the…”
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Simulated non-thermal emission of the supernova remnant G1.9 + 0.3
Published in Monthly notices of the Royal Astronomical Society (09-11-2023)“…ABSTRACT Supernova remnants are the nebular leftover of defunct stellar environments, resulting from the interaction between a supernova blastwave and the…”
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Spectroscopic analysis tool for intEgraL fieLd unIt daTacubEs (satellite): case studies of NGC 7009 and NGC 6778 with MUSE
Published in Monthly notices of the Royal Astronomical Society (26-03-2022)“…ABSTRACT Integral field spectroscopy (IFS) provides a unique capability to spectroscopically study extended sources over a 2D field of view, but it also…”
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Rectangular core-collapse supernova remnants: application to Puppis A
Published in Monthly notices of the Royal Astronomical Society (15-07-2022)“…ABSTRACT Core-collapse supernova remnants are the gaseous nebulae of galactic interstellar media (ISM) formed after the explosive death of massive stars. Their…”
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Discovery of an optical cocoon tail behind the runaway HD 185806
Published in Monthly notices of the Royal Astronomical Society (26-07-2022)“…ABSTRACT Studies on the circumstellar structures around evolved stars provide vital information on the evolution of the parent star and the properties of the…”
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Modelling the interaction of thermonuclear supernova remnants with circumstellar structures: the case of Tycho's supernova remnant
Published in Monthly notices of the Royal Astronomical Society (21-10-2013)“…The well-established Type Ia remnant of Tycho's supernova (SN 1572) reveals discrepant ambient medium-density estimates based on either the measured dynamics…”
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Site-Specific Conjugation of Monomethyl Auristatin E to Anti-CD30 Antibodies Improves Their Pharmacokinetics and Therapeutic Index in Rodent Models
Published in Molecular pharmaceutics (01-06-2015)“…Antibody–drug conjugates (ADCs) have demonstrated clinical benefits that have led to the recent FDA approval of KADCYLA and ADCETRIS. Most ADCs that are…”
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Targeting the immune co-stimulatory molecule CD80 for the imaging of vulnerable atherosclerotic plaques by PET
Published in Atherosclerosis (01-08-2014)Get full text
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Synthesis, characterization and biological evaluation of novel neutral fac-M(CO)3(SNO) complexes (M=Re, 99mTc) bearing the o-methoxyphenylpiperazine moiety
Published in Applied radiation and isotopes (01-06-2012)“…The synthesis, characterization and biological evaluation of two new neutral tricarbonyl fac-M(CO)3(SNO) (M=Re, 99mTc) bearing o-methoxyphenylpiperazine as…”
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Planetary nebulae hosting accreting white dwarfs: A possible solution for the mysterious cut-off of Planetary Nebula Luminosity Function?
Published 14-02-2023“…Many binary companions to the central stars of planetary nebulae (PNe) are found to be inflated, perhaps indicating that accretion onto the central star might…”
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