Winds blowing on a dying star

Eso_20171102_whya_1024

eso_20171102_whya November 9th, 2017

Credit: ALMA (ESO/NAOJ/NRAO), Takigawa et al.

Stars like our Sun constantly eject large amounts of gas and dust into space, but over their lifetimes the levels of this activity change. Scientists continually scour the skies in search of explanations for how and why these changes occur. One such stage of development is the asymptotic giant branch (AGB) near a star's end of life. Dust around these stars plays an important role in regulating stellar winds. This dust is composed of many elements — including metals — which disperse into the galaxy as the winds accelerate. Two such elements are silicon and aluminium. In space, silicon is ten times more abundant than aluminium. However, many oxygen-rich AGB stars are rich in aluminium oxide dust — the source of aluminium — but poor in silicate dust — the source of silicon. This has puzzled researchers: why is aluminium oxide dust so abundant around oxygen-rich AGB stars? A research team led by Aki Takigawa of Kyoto University have utilized a new high spatial-resolution array to obtain and analyse detailed images of the dust surrounding an AGB star. "Previously, there was a limit to how well we could observe stars," explains Takigawa. "Now, thanks to the high spatial resolution of the Atacama Large Millimeter/submillimeter Array, or ALMA, we can obtain images of stars in finer detail. We pointed it toward an aluminium oxide-rich AGB star in the constellation Hydra, W Hydrae." Gas molecules aluminium monoxide and silicon monoxide — AlO and SiO — accelerate around a star, eventually forming aluminium oxide and silicate dust. The team observed that AlO was distributed within three stellar radii of W Hydrae, reflecting the results of previous data. Surprisingly though, SiO was detected beyond five stellar radii, and moreover 70% of these remained gaseous, without forming into dust. "These results indicate that as aluminium oxide accumulates near a star, the addition of a small amount of silicate dust may trigger wind acceleration," elaborates Takigawa. "This decreases gas density, further suppressing silicate dust formation." "This may explain the presence of aluminium-oxide-rich but silicate-poor AGB stars." These results shed light not only on the dynamics of gas and dust surrounding stars, but also on the importance of studying both together. The team plans to continue using ALMA to elucidate gas and dust dynamics in the universe.

Provider: European Southern Observatory

Image Source: https://www.eso.org/public/images/20171102_whya/

Curator: European Southern Observatory, Garching bei München, Germany

Image Use Policy: Creative Commons Attribution 4.0 International License

Image Details

Image Type
Observation
Object Name
W Hydrae
Subject - Milky Way
Star
Eso_20171102_whya_128
 

Position Details

Position (ICRS)
RA = 13h 49m 2.0s
DEC = -28° 22’ 3.5”
Orientation
North is up
Field of View
0.1 x 0.1 arcminutes
Constellation
Hydra

Color Mapping

  Telescope Spectral Band Wavelength
Orange ALMA (Band 7) Millimeter (338 GHZ) 886.0 µm
Spectrum_ir1
Orange
Eso_20171102_whya_1280
×
ID
20171102_whya
Subject Category
B.3  
Subject Name
W Hydrae
Credits
ALMA (ESO/NAOJ/NRAO), Takigawa et al.
Release Date
2017-11-09T00:00:00
Lightyears
Redshift
Reference Url
https://www.eso.org/public/images/20171102_whya/
Type
Observation
Image Quality
Distance Notes
Facility
Atacama Large Millimeter/submillimeter Array
Instrument
Band 7
Color Assignment
Orange
Band
Millimeter
Bandpass
338 GHZ
Central Wavelength
886000
Start Time
Integration Time
Dataset ID
Notes
Coordinate Frame
ICRS
Equinox
J2000
Reference Value
207.258308832, -28.3676303152
Reference Dimension
1048.0, 1036.0
Reference Pixel
524.0, 518.0
Scale
-1.46387429791e-06, 1.46387429791e-06
Rotation
-0
Coordinate System Projection:
TAN
Quality
Full
FITS Header
Notes
Creator (Curator)
European Southern Observatory
URL
http://www.eso.org
Name
Email
Telephone
Address
Karl-Schwarzschild-Strasse 2
City
Garching bei München
State/Province
Postal Code
D-85748
Country
Germany
Rights
Creative Commons Attribution 4.0 International License
Publisher
European Southern Observatory
Publisher ID
eso
Resource ID
20171102_whya
Metadata Date
2017-11-02T15:36:33Z
Metadata Version
1.1
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Detailed color mapping information coming soon...

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There is no distance meta data in this image.

 

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