Unraveling a spiral stream of dusty embers from a massive binary stellar
forge

Date:
September 16, 2020
Source:
National Institutes of Natural Sciences
Summary:
With almost two decades of mid-infrared imaging from the largest
observatories around the world including the Subaru Telescope, a
team of astronomers was able to capture the spiral motion of newly
formed dust streaming from the massive and evolved binary star
system WR112. The study reveals the motion of the dusty outflow
from the system and identifies WR112 as a highly efficient dust
factory that produces an entire Earth mass of dust every year.



FULL STORY ==========================================================================
With almost two decades of mid-infrared (IR) imaging from the largest observatories around the world including the Subaru Telescope, a team of astronomers was able to capture the spiral motion of newly formed dust streaming from the massive and evolved binary star system Wolf-Rayet
(WR) 112.

Massive binary star systems, as well as supernova explosions, are
regarded as sources of dust in the Universe from its early history, but
the process of dust production and the amount of the ejected dust are
still open questions. WR 112 is a binary system composed of a massive
star in the very late stage of stellar evolution losing a large amount
of mass and another massive star at the main sequence. Dust is expected
to be formed in the region where stellar winds from these two stars are colliding. The study reveals the motion of the dusty outflow from the
system and identifies WR 112 as a highly efficient dust factory that
produces an entire Earth mass of dust every year.


==========================================================================
Dust formation, which is typically seen in the gentle outflows from cool
stars with a Sun-like mass, is somewhat unusual in the extreme environment around massive stars and their violent winds. However, interesting things happen when the fast winds of two massive stars in a binary interact.

"When the two winds collide, all Hell breaks loose, including the release
of copious shocked-gas X-rays, but also the (at first blush surprising) creation of copious amounts of carbon-based aerosol dust particles in
those binaries in which one of the stars has evolved to He-burning,
which produces 40% C in their winds," says co-author Anthony Moffat
(University of Montreal). This dust formation process is exactly what
is occurring in WR 112.

This binary dust formation phenomenon has been revealed in other systems
such as WR 104 by co-author Peter Tuthill (University of Sydney). WR 104,
in particular, reveals an elegant trail of dust resembling a 'pinwheel'
that traces the orbital motion of the central binary star system.

However, the dusty nebula around WR 112 is far more complex than a simple pinwheel pattern. Decades of multi-wavelength observations presented conflicting interpretations of the dusty outflow and orbital motion of
WR 112.

After almost 20 years uncertainty on WR 112, images from the COMICS
instrument on the Subaru Telescope taken in Oct 2019 provided the final --
and unexpected -- piece to the puzzle.

"We published a study in 2017 on WR 112 that suggested the dusty nebula
was not moving at all, so I thought our COMICS observation would confirm
this," explained lead author Ryan Lau (ISAS/JAXA). "To my surprise, the
COMCIS image revealed that the dusty shell had definitely moved since
the last image we took with the VLT in 2016. It confused me so much that
I couldn't sleep after the observing run -- I kept flipping through the
images until it finally registered in my head that the spiral looked
like it was tumbling towards us." Lau collaborated with researchers at
the University of Sydney including Prof.

Peter Tuthill and undergraduate Yinuo Han, who are experts at modeling
and interpreting the motion of the dusty spirals from binary systems
like WR 112.

"I shared the images of WR 112 with Peter and Yinuo, and they were able to produce an amazing preliminary model that confirmed that the dusty spiral stream is revolving in our direction along our line of sight," said Lau.

The animation above shows a comparison between the models of WR 112
created by the research team alongside the actual mid-IR observations. The appearance of the model images shows a remarkable agreement with the
real images of WR 112.

The models and the series of imaging observations revealed that the
rotation period of this dusty "edge-on" spiral (and the orbital period
of the central binary system) is 20 years.

With the revised picture of WR 112, the research team was able to
deduce how much dust this binary system is forming. "Spirals are
repetitive patterns, so since we understand how much time it takes to
form one full dusty spiral turn (~20 years), we can actually trace the
age of dust produced by the binary stars at the center of the spiral,"
says Lau. He points out that "there is freshly formed dust at the very
central core of the spiral, while the dust we see that's 4 spiral turns
away is about 80 years old. Therefore, we can essentially trace out
an entire human lifetime along the dusty spiral stream revealed in our observations. So I could actually pinpoint on the images the dust that
was formed when I was born (right now, it's somewhere in between the
first and second spiral turns)." To their surprise, the team found WR
112 is a highly efficient dust factory that outputs dust at a rate of
3x10-6 solar mass per year, which is equivalent to producing an entire
Earth mass of dust every year. This was unusual given WR 112's 20-yr
orbital period -- the most efficient dust producers in this type of WR
binary star system tend to have shorter orbital periods less than a year
like WR 104 with its 220-day period. WR 112 therefore demonstrates the diversity of WR binary systems that are capable of efficiently forming
dust and highlights their potential role as significant sources of dust
not only in our Galaxy but galaxies beyond our own.

Lastly, these results demonstrate the discovery potential of multi-epoch
mid-IR imaging with the MIMIZUKU instrument on the upcoming Tokyo Atacama Observatory (TAO). The mid-IR results from this study notably utilize
the largest observatories in the world and set the stage for the next
decade of astronomical discoveries with 30-m class telescopes and the
upcoming James Webb Space Telescope.


========================================================================== Story Source: Materials provided by
National_Institutes_of_Natural_Sciences. Note: Content may be edited
for style and length.


========================================================================== Journal Reference:
1. Ryan M. Lau, Matthew J. Hankins, Yinuo Han, Izumi Endo, Anthony
F. J.

Moffat, Michael E. Ressler, Itsuki Sakon, Joel Sanchez-Bermudez,
Anthony Soulain, Ian R. Stevens, Peter G. Tuthill, Peredur
M. Williams. Resolving Decades of Periodic Spirals from the
Wolf-Rayet Dust Factory WR 112. The Astrophysical Journal, 2020;
900 (2): 190 DOI: 10.3847/1538-4357/abaab8 ==========================================================================

Link to news story: https://www.sciencedaily.com/releases/2020/09/200916094243.htm

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