[HTML][HTML] Overview of non-transient γ-ray binaries and prospects for the Cherenkov Telescope Array

M Chernyakova, D Malyshev, A Paizis… - Astronomy & …, 2019 - aanda.org
Aims. Despite recent progress in the field, there are still many open questions regarding γ-
ray binaries. In this paper we provide an overview of non-transient γ-ray binaries and …

Distinguishing circumstellar from stellar photometric variability in Eta Carinae

A Damineli, E Fernández-Lajús… - Monthly Notices of …, 2019 - academic.oup.com
ABSTRACT The interacting binary Eta Carinae remains one of the most enigmatic massive
stars in our Galaxy despite over four centuries of observations. In this work, its light curve …

Simulating the response of the secondary star of Eta Carinae to mass accretion at periastron passage

A Kashi - Monthly Notices of the Royal Astronomical Society, 2019 - academic.oup.com
We use high-resolution 3D hydrodynamical simulations to quantify the amount of mass
accreted on to the secondary star of the binary system Eta Carinae, exploring two sets of …

η Carinae: Particle acceleration and multimessenger aspects

R Walter, M Balbo - Astronomische Nachrichten, 2019 - Wiley Online Library
η Carinae is composed of two very massive stars orbiting each other in 5.5 years. The
primary star features the densest known stellar wind, colliding with that expelled by its …

[PDF][PDF] Diffusive shock acceleration and the resulting non-thermal emission from colliding-wind binary systems

JM Pittard, GS Vila, GE Romero - arXiv, 2019 - researchgate.net
We present a new model for the non-thermal emission from a colliding-wind binary.
Relativistic protons and electrons are assumed to be accelerated through diffusive shock …

Gamma-rays and positrons from Colliding Wind Binaries

M Balbo, R Walter - arXiv preprint arXiv:1909.00793, 2019 - arxiv.org
The $\eta $ Carinae binary system is the first $\gamma $-ray binary ever observed which
does not contain a compact object. The dense wind of the primary star shocks against the …

[PDF][PDF] Distinguishing circumstellar from stellar photometric variability in Eta CarinaeQ2:[Copyeditor to Author][Author: The

A Damineli - researchgate.net
ABSTRACT The interacting binary Eta Carinae remains one of the most enigmatic massive
stars in our Galaxy despite over four centuries of observations. In this work, its light curve …

[引用][C] Super-Hard X-Ray Emission from Carinae Observed with Suzaku

A SEKIGUCHI, M TSUJIMOTO, S KITAMOTO