ALMA reveals a strikingly beautiful view of a delicate bubble of expelled material around the exotic red star U Antliae, helping astronomers to better understand how stars evolve during the later stages of their life cycles.
In the faint southern constellation of Antlia (The Air Pump) the careful observer with binoculars will spot a very red star, which varies slightly in brightness from week to week. This very unusual star is called U Antliae and new observations with the Atacama Large Millimeter/submillimeter Array (ALMA) are revealing a remarkably thin spherical shell around it.
U Antliae is a carbon star, an evolved, cool, and luminous star of the asymptotic giant branch type. Around 2700 years ago, U Antliae went through a short period of rapid mass loss. During this period of only a few hundred years, the material making up the shell seen in the new ALMA data was ejected at high speed. Examination of this shell in further detail also shows some evidence of thin, wispy gas clouds known as filamentary substructures.
This spectacular view was only made possible by the unique ability to create sharp images at multiple wavelengths that is provided by the ALMA radio telescope, located on the Chajnantor Plateau in Chile’s Atacama Desert. ALMA can see a much finer structure in the U Antliae shell than has previously been possible.
The new ALMA data are not just a single image; ALMA produces a three-dimensional dataset (a data cube) with each slice being observed at a slightly different wavelength. Because of the Doppler Effect, this means that different slices of the data cube show images of gas moving at different speeds toward or away from the observer. This shell is also remarkable as it is very symmetrically round and also remarkably thin. By displaying the different velocities we can cut this cosmic bubble into virtual slices just as we do in computer tomography of a human body.
Understanding the chemical composition of the shells and atmospheres of these stars, and how these shells form by mass loss, is important to properly understand how stars evolve in the early Universe and also how galaxies evolved. Shells such as the one around U Antliae show a rich variety of chemical compounds based on carbon and other elements. They also help to recycle matter and contribute up to 70% of the dust between stars.
The data collected with ALMA are not just a single image, but a three-dimensional dataset (a data cube) with each slice being observed at a slightly different wavelength. Because of the Doppler effect, different slices of the data cube show images of gas moving at different speeds toward or away from the observer. By displaying different velocities we can cut this cosmic bubble into virtual slices just as we do in computer tomography of a human body. Credit: ALMA (ESO/NAOJ/NRAO)/F. Kerschbaum
Reference: “Rings and filaments: The remarkable detached CO shell of U Antliae” by F. Kerschbaum, M. Maercker, M. Brunner, M. Lindqvist, H. Olofsson, M. Mecina, E. De Beck, M. A. T. Groenewegen, E. Lagadec, S. Mohamed, C. Paladini, S. Ramstedt, W. H. T. Vlemmings and M. Wittkowski, 3 August 2018, Astronomy & Astrophysics.
DOI: 10.1051/0004-6361/201730665
PDF
Never miss a breakthrough: Join the SciTechDaily newsletter.
Follow us on Google and Google News.