Novae II. Model, multi-band outburst, bipolar ejecta, accretion disk, relativistic electrons, etc
Nimisha Kantharia (National Centre for Radio Astrophysics, Tata, Institute of Fundamental Research, Pune)

TL;DR
This paper presents a comprehensive physical model for classical and recurrent novae, emphasizing relativistic electrons, bipolar ejecta, and the role of rotation and accretion in nova outbursts based on multi-wavelength observations.
Contribution
It introduces a self-consistent model explaining nova phenomena, including relativistic electron energization, bipolar ejecta formation, and the influence of rotation on accretion and outflows.
Findings
Electrons are energized to relativistic velocities during explosion without shock acceleration.
Rotation causes latitude-dependent accretion, leading to bipolar ejecta.
Accretion disks form around rotating objects, not non-rotating ones.
Abstract
The study of novae is continued and a self-consistent updated physical model for classical/recurrent novae derived from multi-wavelength observations is presented. In particular, observations of novae support the origin of the optical continuous emission in the outburst ejecta, mass-based segregation and clump formation in the ejecta, origin of the Orion, diffuse enhanced lines and dust in the clumps, prompt Fe II line formation in swept-up material, energising of electrons to relativistic velocities by the explosion and the existence of a large cool envelope around the accreting white dwarf in quiescence. The rapid transfer of thermonuclear energy should be adiabatic which energises and ejects all the particles in the overlying layers. Our study results in the following conclusions which are relevant for novae and other astrophysical systems: (1) Electrons are instantaneously energised…
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Taxonomy
TopicsAstrophysical Phenomena and Observations · Diamond and Carbon-based Materials Research · Atomic and Molecular Physics
