CO, Water, and Tentative Methanol in η Carinae Approaching Periastron

PW Morris, SB Charnley, M Corcoran… - The Astrophysical …, 2020 - iopscience.iop.org
The complex circumstellar environment around the massive binary and luminous blue
variable η Carinae is known to harbor numerous light molecules, emitting most strongly in …

Onthe changes in the physical properties of the ionized region around the Weigelt structures in η Carinae over the 5.54-yr spectroscopic cycle

M Teodoro, TR Gull, MA Bautista… - Monthly Notices of …, 2020 - academic.oup.com
We present HST/STIS observations and analysis of two prominent nebular structures around
the central source of η Carinae, the knots C and D. The former is brighter than the latter for …

Wind collision and accretion simulations of the massive binary system HD 166734

A Kashi - Monthly Notices of the Royal Astronomical Society, 2020 - academic.oup.com
ABSTRACT I have run hydrodynamic simulations that follow the colliding wind structure of
the massive binary system HD 166734 along its binary orbit. I show that close to periastron …

[图书][B] A Three Dimensional Adaptive Mesh Refinement Hydrodynamical Simulation of Eta Carinae's Colliding Stellar Winds around Periastron

TP Ho - 2020 - search.proquest.com
One of the most luminous and mysterious binary star systems, classified as a Luminous Blue
Variable (LBV), is known to astronomers as Eta Carinae. Located 7,500 light years away …

[PDF][PDF] ACCRETION SIMULATIONS OF η CARINAE AND IMPLICATIONS FOR THE EVOLUTION OF MASSIVE BINARIES

C Neiner, WW Weiss, D Baade, RE Griffin, CC Lovekin - starsandspace.univie.ac.at
This contribution presented high-resolution numerical simulations of the colliding wind
system η Carinae, showing accretion of the primary wind onto the secondary star close to …