Ring of Stars in Centaurus A Uncovered
Written by Nicholos Wethington
Centaurus A (NGC 5128) is one of the most studied objects in the Southern sky, because it is the giant elliptical galaxy with the closest proximity to our own Milky Way. It lies 11 million light years away from the Milky Way, and is believe to have merged with another gaseous galaxy about 200 to 700 million years ago. The result of this galactic mashup: the birth of hundreds of thousands of stars in a kiloparsec-spanning ring near the core.
This is the first time that the inner structure of the galaxy has been resolved in such detail. Using the SOFI large field Infra-Red (1-2.5 micron) spectro-imager at the ESO New Technology Telescope, a research team led by Jouni Kainulainen of the University of Helsinki and Max Planck Institute for Astronomy was able to image a large ring of stars that have formed – and are still continuing to form – near the center of the galaxy. The brightest sources in the ring are red supergiants, or low-mass star clusters.
"It is important to note that it is not decisively the instrument (the telescope or the instrument attached to it) that enables us to see through dust, but the data analysis technique that is used to analyze the images taken with it. Of course, the instrument plays a big role in a sense that adequately high-quality images are needed to perform the analysis," Dr. Kainulainen said in an email interview.
"There is a fundamental difference between the images we use in our paper and the Spitzer images: the wavelength that the images cover. In the images we used in our work, the dust lane of Centaurus A shows itself as "a shadow", or more precisely, as an absorption feature (the wavelength is 1-2 micrometers). The Spitzer images represent somewhat longer wavelengths, and show the radiation emitted by the dust itself. As a concrete example, the most famous Spitzer image of Centaurus A … shows a parallelogram-like structure, but the image describes radiation mainly from dust, not from stars," he said.
There is a large, S- or bar-shaped dust lane straight through the center of Centaurus A that obscures observations in the visible light spectrum. As shown in the image below, the ring structure of star formation is obscured by dust, but visible in the near-infrared.
Centaurus A is believe to house a supermassive black hole that has the mass of 200 million Suns at its core, evidenced by the radio emissions streaming out from the galaxy. Previous images of the galaxy from the Spitzer Space Telescope, the ESA's Infrared Space Observatory and the Hubble Space Telescope revealed some aspects of the structure of the galaxy. The infrared eyes of Spitzer peered partway through the dust to show a warped parallelogram, the cause of which is the gravitational disturbance caused by the merger of Centaurus A with a smaller spiral galaxy.
The presence of rings such as the one seen in Centaurus A is probably not common among other elliptical galaxies, but other such galaxies are known to exist. It's possible that they are present during only certain periods of an elliptical galaxy's formation after it merges with another galaxy.
Dr. Kainulainen commented on this possiblity: "One should consider that seeing so bright ring structure is probably quite time-critical. The rings are believed to be induced by "a violent event" of merging galaxies, and they may evolve rather quickly to something that no longer looks like a clear, bright ring. Therefore, they might actually be quite common for merging galaxies, but they "last" only such a short time that we don't see them in so many galaxies."
The analysis technique used by the team could be applied to other galaxies to resolve formation structures previously hidden by dust, and provide more information about how violent events alter the formation of elliptical galaxies.
"Potentially, the technique can be applied to any relatively nearby galaxy showing prominent dust features. Such targets could be M31, M83, M51, Fornax A, or any similarly large, bright, dust containing galaxy. Due to geometrical reasons, Centaurus A was a very suitable target for applying the method. It will be more challenging in the case of, for example, normal Spiral galaxies. However, we have already experimented with such galaxies and feel positive about the possibilities they give," said Dr. Kainulainen.
The striking image of Centaurus A's ring of star formation was a somewhat surprising result of the imaging that the astronomers took of the galaxy, though there were hints from images taken by other telescopes that stellar formation was present in the obscured, dusty core.
Dr. Kainulainen said, "It was very surprising that the structure contained so much stars and star-forming activity, and that we could reveal it in such great detail. However, it was expected that a structure of this kind exists there, and contains at least some star formation. This was evident, for example, from the earlier Spitzer images. But when I first saw our result, "The Naked Picture of Centaurus A", on my computer screen, it really was a big WOW-feeling!"
Further observations of Centaurus A are definitely in order to further explore the structure of the stellar ring, and the gravitational dynamics that allowed for its formation.
"Our plans include observations with the Very Large Telescope (European Southern Observatory) and the Hubble Space Telescope. In that work, the information we got about the dust lane in our published Letter will play a significant role. The planned observations aim particularly at determining how long, and in what magnitude, the structure has been forming stars in the past. Such information will help to understand galaxy-merging process, which is not an uncommon event in the Universe.
Dr. Kainulainen and his team published their results in a letter to Astronomy & Astrophysics, published online July 2nd, 2009. The full text of the letter is available here.
Source: ESO, Astronomy and Astrophysics, email interview with Jouni Kainulainen
Filed under: galaxies
Tags: centaurus A, near-infrared astronomyRelated stories on Universe Today
Comment policy: Be nice and brief. Don't advertise your stuff, or promote your personal theories. We'll delete any comments that break these policies. Click here for more details.
November 22nd, 2009 at 7:27 pm
Part of "The many faces of Centaurus A" ( http://www.atnf.csiro.au/research/cena/gallery_showimage.php?i=08 ).
November 23rd, 2009 at 1:42 am
Eerie.
November 23rd, 2009 at 7:11 am
I am not a galaxy structure maven, but it is my understanding that rings like this are similar to a hydrodynamic wave or splash signifying some past event that unleashed energy. Of course to do this across a whole galaxy requires a lot of energy.
LC
November 23rd, 2009 at 7:22 am
This is fascinating.
What if all elliptical galaxies are just large galactic cores and they all have a spiral of stars surrounding them?
I like to see more ellipticals resolved to this level of detail.
November 23rd, 2009 at 8:11 am
Jon Hanford is more of a galaxy structure and observational sort, so you might confer with him on the nature of elliptical galaxies. It is my understanding that elliptical galaxies may result from the coalescence of smaller galaxies, which might presumably involve spiral galaxies. The Milky Way and Andromeda galaxies are going to coalesce in 2.5 billion years or so, and will probably setting into some form of elliptical galaxy (the Andromilkaway galaxy?).
LC
November 23rd, 2009 at 2:18 pm
@ Lawrence Crowell, I'm not sure if Centaurus A would be considered a classical ring galaxy, but perhaps may be related to polar ring galaxies (which are thought to form through a different process than ring galaxies). But, no doubt, a small fuel-rich galaxy (probably some type of spiral or disk galaxy) is being accreted onto the elliptical. Some of the dust and gas from this galaxy probably contributed material that we see as a ring of stars 30,000 l.y.(1 kpc) from the nucleus. As mentioned in the article, the ring is probably a 'short-lived' phenomena compared to the life of a galaxy.
@ Spoodle58, some elliptical galaxies do exhibit 'stellar rings' around their nuclei, although these rings are usually seen much closer to the nucleus and have a younger stellar component. You mention the detail seen in these images and I, too, would like to 'see more ellipticals resolved to this level of detail', but this is partly a function of distance. Centarus A is truly a massive, active galaxy that just happens to lie nearby. Compared to other radio galaxies like M 87 or NGC 1275, Cen A is practically in our backyard, so we can explore its active nucleus and bipolar jet in exquisite detail. Centaurus A is one of the few galaxies known to exhibit jet-induced star formation.
November 23rd, 2009 at 2:44 pm
Spitzer infrared observations of the warped ring in Cen A can be found here: http://arxiv.org/PS_cache/astro-ph/pdf/0601/0601135v1.pdf . Although Spitzer observed at slightly longer wavelengths (3.6 to 8 microns) as opposed to the JHK images presented here, it makes for an interesting comparison. This paper also describes modeling of the warped disk component.
November 23rd, 2009 at 4:11 pm
Am i missing something? My understanding is that Andromeda is about 2.5 megalights from us and we will smash together in about 3-3.5 billion years from now, but how does Centarus become the closest galaxy when it is 11 megalights away?
November 23rd, 2009 at 4:30 pm
For santafedog
Closest Giant elliptical galaxy is Centarus A and yes Andromeda is the closest large spiral galaxy, that we know of. Also there are lots of small galaxies closer again, like the LMC and the SMC.
For Jon Hanford
I understand the distances involved, I meant more detail as in bigger and better telescopes/spacecraft etc. And also it would be interesting to see if all elliptical galaxies had a spiral ring around them, maybe all galaxies are spiral in structure. Food for thought.
November 23rd, 2009 at 4:32 pm
Jon thanks for that. It might also be that the large BH at the center is playing some sort of role. I have seen simulations which do predict ring galaxies after collisions. I think these are usually due to the impact of a small galaxy normal to the disk of the larger one.
LC