ESA Science & Technology - Hubble traces the halo of a galaxy more accurately than ever before [heic1415]

Centaurus A halo. Image Credit: ESA/Hubble, NASA, Digitized Sky Survey, MPG/ESO. Acknowledgement: Davide de Martin

There is more to a galaxy than first meets the eye. Extending far beyond the bright glow of a galaxy's centre, the swirling spiral arms, or the elliptical fuzz, is an extra component: a dim halo of stars sprawling into space.

These expansive haloes are important components of a galaxy. The halo of our own galaxy, the Milky Way, preserves signatures of both its formation and evolution. Yet, we know very little about the haloes of galaxies beyond our own as their faint and spread-out nature makes exploring them more difficult. Astronomers have so far managed to detect very few starry haloes around other galaxies.

Now, by utilising the unique space-based location of the NASA/ESA Hubble Space Telescope and its sensitive Advanced Camera for Surveys and Wide Field Camera 3, a team of astronomers has probed the halo surrounding the prominent giant elliptical galaxy Centaurus A [1], also known as NGC 5128, to unprecedented distances. They have found that its halo spreads far further into space than expected and does so in an unexpected form.

"Tracing this much of a galaxy's halo gives us surprising insights into a galaxy's formation, evolution, and composition," says Marina Rejkuba of the European Southern Observatory in Garching, Germany, lead author of the new Hubble study. "We found more stars scattered in one direction than the other, giving the halo a lopsided shape – which we hadn't expected!"

Along the galaxy's length the astronomers probed out 25 times further than the galaxy's radius – mapping a region some 450 000 light-years across. For the width they explored along 295 000 light-years, 16 times further than its "effective radius" [2]. These are large distances if you consider that the main visible component of the Milky Way is around 120 000 light-years in diameter. In fact, the diameter of the halo probed by this team extends across 4 degrees in the sky – equivalent to eight times the apparent width of the Moon.

Alongside their unexpected uneven distribution, the stars within the halo also showed surprising properties relating to the proportion of elements heavier than hydrogen and helium found in the gas that makes up the stars. While the stars within the haloes of the Milky Way and other nearby spirals are generally low in heavy elements, the stars within Centaurus A's halo appear to be rich in heavy elements, even at the outermost locations explored.

"Even at these extreme distances, we still haven't reached the edge of Centaurus A's halo, nor have we detected the very oldest generation of stars," adds co-author Laura Greggio of INAF, Italy. "This aged generation is very important. The larger stars from it are responsible for manufacturing the heavy elements now found in the bulk of the galaxy's stars. And even though the large stars are long dead, the smaller stars of the generation still live on and could tell us a great deal."

The small quantity of heavy elements in the stellar haloes of large spiral galaxies like the Milky Way, is thought to originate from the way that the galaxies formed and evolved, slowly pulling in numerous small satellite galaxies and taking on their stars. For Centaurus A, the presence of stars rich in heavy elements in such remote locations suggests a single past merger with a large spiral galaxy. This event would have ejected stars from the spiral galaxy's disc and these are now seen as part of Centaurus A's outer halo.

"Measuring the amount of heavy elements in individual stars in a giant elliptical galaxy such as Centaurus A is uniquely the province of Hubble – we couldn't do it with any other telescope, and certainly not yet from the ground," adds Rejkuba. "These kinds of observations are fundamentally important to understanding the galaxies in the Universe around us."

These results are being published online in Astrophysical Journal on the 22 July and will appear in the 10 August 2014 issue.

Notes

[1] As it is relatively near to Earth, Centaurus A is prominent in our night sky and is well known for its striking and beautiful appearance (heic1110, opo9814e). To see more about this galaxy, see Hubblecast 46: A tour of Centaurus A.

[2] The effective radius of a galaxy, as referenced here, is the radius of the area in which half of the galaxy's light is emitted. Astronomers use this effective radius rather than the full radius because the galaxy becomes faint and undefined at its outskirts.

More information

The Hubble Space Telescope is a project of international cooperation between ESA and NASA.

The international team of astronomers in this study consists of M. Rejkuba (European Southern Observatory, Germany; Excellence Cluster Universe, Germany), W. E. Harris (McMaster University, Canada), L. Greggio (INAF, Italy), G. L. H. Harris (University of Waterloo, Canada), H. Jerjen (Australian National University, Australia), O. A. Gonzalez (European Southern Observatory, Chile).

Contacts

Marina Rejkuba
European Southern Observatory
Garching bei München, Germany
Tel: +49 89 3200 6453
Cell: +49 151 21259320
Email: mrejkubaeso.org

Laura Greggio
INAF, Osservatorio Astronomico di Padova
Padova, Italy
Tel: +39 049 8293463
Cell: +39 347 73189089
Email: laura.greggiooapd.inaf.it

Georgia Bladon
ESA/Hubble, Public Information Officer
Garching bei München, Germany
Cell: +44 7816291261
Email: gbladonpartner.eso.org