Analytical approximations and 2D hydrodynamical simulations are used to examine the interaction of supernova fragments with the internal structure of large...
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PublicationThe impact of supernova fragments on the evolution of multisupernova remnants
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PublicationThe interstellar medium in the Upper Cepheus-Cassiopeia region
We have studied the kinematics and spatial distribution of the interstellar gas in the sky region 110°
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TalkThe jet feedback mechanism: from supernovae to clusters of galaxies
I will describe the roles of jets in several quite different astrophysical systems. These include exploding core collapse supernovae, expelling common envelopes...
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PublicationThe spectrum and evolution of compact SNR: SN and AGN.
The evolution and spectra from a compact supernova remnant evolving in a high-density circumstellar medium with a density of 107cm-3 are presented. The...
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PublicationThe starburst model for active galactic nuclei - The broad-line region as supernova remnants evolving in a high-density medium
The evolution of an SNR in a high-density medium has been studied using analytical and numerical hydrodynamic and photoionization models. The models show that...
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PublicationThin shell formation in radiative shocks. 1: Supernova remnants in low-density media
This paper explores the onset of thin-shell formation in interstellar shocks associated with supernova explosions. We outline a simple but useful scheme that...
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PublicationThree supernova shells around a young M33 star cluster
Using a specialized technique sensitive to the presence of expanding ionized gas, we have detected a set of three concentric expanding shells in an H II region...
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PublicationVery energy observations of PSR B1951+32
PSR B1951+32 is a γ-ray pulsar detected by the Energetic Gamma Ray Experiment Telescope (EGRET) and identified with the 39.5 ms radio pulsar in the supernova...
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PublicationVery High Energy Observations of PSR B1951+32
PSR B1951+32 is a gamma -ray pulsar detected by the Energetic Gamma Ray Experiment Telescope (EGRET) and identified with the 39.5 ms radio pulsar in the...