output
20152026
most citedTwo dimensional magnets: Forgotten history and recent progress towards spintronic applications

234 citations

Showing 2020 · astro-ph.HEShow all

12 papers · 2 filters

astro-ph.HE2020★ 22 cited

A pre-explosion extended effervescent zone around core collapse supernova progenitors

Noam Soker

I propose a scenario according to which the dense compact circumstellar matter (CSM) that the ejecta of many core collapse supernovae (CCSNe) collide with within several days after…

astro-ph.HE2020★ 3 cited

Possible post-kick jets in SN 1987A

Noam Soker

I suggest that the recently observed hot-dust elongated structure that likely engulfs the neutron star (NS) remnant of supernova (SN) 1987A was shaped by jets that the NS launched…

astro-ph.HE2020★ 9 cited

The circumstellar matter of type II intermediate luminosity optical transients (ILOTs)

Noam Soker

I find that a 0.1-1Mo outflowing equatorial dusty disk (torus) that the binary system progenitor of an intermediate luminosity optical transient (ILOT) ejects several years to seve…

astro-ph.HE2020★ 7 cited

The X-ray properties of Eta Carinae during its 2020 X-ray minimum

Amit Kashi, David A. Principe, Noam Soker +1

The massive binary system Eta Carinae is characterized by intense colliding winds that form shocks and emit X-rays. The system is highly eccentric (), resulting in modu…

astro-ph.HE2020★ 11 cited

Simulating jets from a neutron star companion hours after a core collapse supernova

Muhammad Akashi, Noam Soker

We conduct three-dimensional hydrodynamical simulations to explore the interaction of jets that a neutron star (NS) companion to a type Ic or type Ib core collapse supernova (CCSN)…

astro-ph.HE2020★ 5 cited

Modelling light curves of bipolar core collapse supernovae from the equatorial plane

Noam Soker, Noa Kaplan

We use the two-components bipolar toy model of core collapse supernova (CCSN) ejecta to fit the rapid decline from maximum luminosity in the light curve of the type IIb CCSN SN 201…

astro-ph.HE2020★ 17 cited

Explaining recently studied intermediate luminosity optical transients (ILOTs) with jet powering

Noam Soker, Noa Kaplan

We apply the jet-powered ILOT scenario to two recently studied intermediate luminosity optical transients (ILOTs), and find the relevant shell mass and jets' energy that might acco…

astro-ph.HE2020★ 10 cited

Simulating the inflation of bubbles by late jets in core collapse supernova ejecta

Muhammad Akashi, Noam Soker

We conducted three-dimensional hydrodynamical simulations to study the interaction of two late opposite jets with the ejecta of a core collapse supernova (CCSN), and study the bipo…

astro-ph.HE2020★ 5 cited

Minutes-delayed jets from a neutron star companion in core collapse supernovae

Noam Soker

I study cases where a neutron star (NS; or a black hole) companion to a type Ib or type Ic (stripped-envelope) core collapse supernova (CCSN) accretes mass from the explosion eject…

astro-ph.HE2020★ 5 cited

Eccentric grazing envelope evolution towards type IIb supernova progenitors

Dmitry Shishkin, Noam Soker

We simulate the evolution of eccentric binary systems in the frame of the grazing envelope evolution (GEE) channel for the formation of Type IIb supernovae (SNe IIb), and find that…

astro-ph.HE2020★ 14 cited

Jet-shaped geometrically modified light curves of core collapse supernovae

Noa Kaplan, Noam Soker

We build three simple bipolar ejecta models for core collapse supernovae (CCSNe), as expected when the explosion is driven by strong jets, and show that for an observer located in…

astro-ph.HE2020★ 35 cited

Efficiently jet-powered radiation in intermediate-luminosity optical transients (ILOTS)

Noam Soker

I show that a flow structure where wide jets hit a slower expanding shell might be very efficient in channelling the kinetic energy of the jets to radiation, therefore accounting f…