Zobrazeno 1 - 7
of 7
pro vyhledávání: '"Chiotellis, Alexandros"'
Autor:
Derlopa, Sophia, Akras, Stavros, Amram, Philippe, Boumis, Panos, Chiotellis, Alexandros, de Oliveira, Claudia Mendes
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 and a knotty central region. We performed an upgrated 3D Morpho-kinem
Externí odkaz:
http://arxiv.org/abs/2405.00169
Mixed-morphology supernova remnants (MMSNRs) are characterized by a shell-like morphology in the radio and centrally-peaked thermal emission in the X-ray band. The nature of this peculiar class of supernova remnants (SNRs) remains a controversial iss
Externí odkaz:
http://arxiv.org/abs/2403.19743
Autor:
Arias, Maria, Zhou, Ping, Chiotellis, Alexandros, De Breuck, Carlos, Domcek, Vladimir, Boumis, Panos, Vink, Jacco, Derlopa, Sophia, Akras, Stavros
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 350.0-2.0, that look remarkably similar in continuum radio emission, showing
Externí odkaz:
http://arxiv.org/abs/2402.10763
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 astrophysical code SHAPE in which wide field imaging and high resolution spectr
Externí odkaz:
http://arxiv.org/abs/2008.04958
The first 3D Morpho-kinematical model of a Supernova Remnant: The case of VRO 42.05.01 (G 166.0+4.3)
We present the preliminary results of the first 3-dimensional (3D) Morpho-Kinematical (MK) model of a supernova remnant (SNR), using as a study case the Galactic SNR VRO 42.05.01 (G 166.0+4.3). For the purpose of our modelling, the astrophysical soft
Externí odkaz:
http://arxiv.org/abs/1909.06131
We present the results of a detailed investigation of the Galactic supernova remnant RCW 86 using the XMM-Newton X-ray telescope. RCW 86 is the probable remnant of SN 185 A.D, a supernova that likely exploded inside a wind-blown cavity. We use the XM
Externí odkaz:
http://arxiv.org/abs/1404.5434
One of the key observables for determining the progenitor nature of Type Ia supernovae is provided by their immediate circumstellar medium, which according to several models should be shaped by the progenitor binary system. So far, X-ray and radio ob
Externí odkaz:
http://arxiv.org/abs/1401.7332