The spectacular aftermath of a 360 million year old cosmic collision is revealed in great detail in new images from ESOâ€™s Very Large Telescope at the Paranal Observatory. Among the debris is a rare and mysterious young dwarf galaxy. This galaxy is providing astronomers with an excellent opportunity to learn more about similar galaxies that are expected to be common in the early Universe, but are normally too faint and distant to be observed by current telescopes.
NGC 5291, the hazy, golden oval dominating the centre of this image, is an elliptical galaxy located nearly 200 million light-years away in the constellation of Centaurus (The Centaur). Over 360 million years ago, NGC 5291 was involved in a dramatic and violent collision as another galaxy travelling at immense speeds barrelled into its core. The cosmic crash ejected huge streams of gas into nearby space, which later coalesced into a ring formation around NGC 5291 .
Over time, material in this ring gathered and collapsed into dozens of star-forming regions and several dwarf galaxies, revealed as pale blue and white regions scattered around NGC 5291 in this new image from the FORS instrument, mounted on the VLT. The most massive and luminous clump of material, to the right of NGC 5291, is one of these dwarf galaxies and is known as NGC 5291N.
The Milky Way, like all large galaxies, is believed to have formed through the build-up of smaller dwarf galaxies in the early years of the Universe. These small galaxies, if they have survived on their own up to the present day, now normally contain many extremely old stars.
Yet NGC 5291N appears to contain no old stars. Detailed observations with the MUSE spectrograph  also found that the outer parts of the galaxy had properties typically associated with the formation of new stars, but what was observed is not predicted by current theoretical models. Astronomers suspect that these unusual aspects may be the result of massive collisions of gas in the region.
NGC 5291N doesnâ€™t look like a typical dwarf galaxy, but instead it shares a striking number of similarities with the clumpy structures present within many of the star-forming galaxies in the distant Universe. This makes it a unique system in our local Universe and an important laboratory for the study of early gas-rich galaxies, which are normally much too distant to be observed in detail by current telescopes.
This unusual system has previously been observed by a wide range of ground-based facilities, including ESOâ€™s 3.6-metre telescope at the La Silla Observatory . However, the capabilities of MUSE, FORS and the Very Large Telescope have only now allowed some of the history and properties of NGC 5291N to be determined.
Future observations, including those by ESOâ€™s European Extremely Large Telescope (E-ELT), may allow astronomers to further unravel this dwarf galaxyâ€™s remaining mysteries.
Notes NGC 5291 is currently also interacting more gently with MCG-05-33-005 â€” or the Seashell Galaxy â€” the unusual comma-shaped galaxy appearing to leech off NGC 5291â€™s luminous core.  NGC 5291N was observed using integral field spectrography during MUSEâ€™s first Science Verification run. Integral field spectrography collects a spectrum at every point on the sky, providing a powerful three-dimensional view of the target. The MUSE observations revealed unexpected oxygen and hydrogen emission lines in the outskirts of NGC 5291N.  NGC 5291 was studied by astronomers using ESOâ€™s 3.6-metre telescope at the La Silla Observatory back in 1978. These observations revealed large amounts of material in the intergalactic space around the galaxy, which we now know to be the star-forming regions and several dwarf galaxies created from the collapse of the galaxyâ€™s gaseous ring.
This research was presented in a paper entitled â€œIonization processes in a local analogue of distant clumpy galaxies: VLT MUSE IFU spectroscopy and FORS deep images of the TDG NGC 5291Nâ€, by J. Fensch et al., to appear in the journal Astronomy Astrophysics.
The team is composed of J. Fensch (Laboratoire AIM Paris-Saclay, CEA/IRFU/SAp, Universite Paris Diderot, Gif-sur-Yvette, France [CEA]), P.-A. Duc (CEA) , P. M. Weilbacher (Leibniz-Institut fÃ¼r Astrophysik, Potsdam, Germany), M. Boquien (University of Cambridge, United Kingdon; Universidad de Antofagasta, Antofagasta, Chile) and E. Zackrisson (Uppsala University, Uppsala, Sweden).
ESO is the foremost intergovernmental astronomy organisation in Europe and the worldâ€™s most productive ground-based astronomical observatory by far. It is supported by 16 countries: Austria, Belgium, Brazil, the Czech Republic, Denmark, France, Finland, Germany, Italy, the Netherlands, Poland, Portugal, Spain, Sweden, Switzerland and the United Kingdom, along with the host state of Chile. ESO carries out an ambitious programme focused on the design, construction and operation of powerful ground-based observing facilities enabling astronomers to make important scientific discoveries. ESO also plays a leading role in promoting and organising cooperation in astronomical research. ESO operates three unique world-class observing sites in Chile: La Silla, Paranal and Chajnantor. At Paranal, ESO operates the Very Large Telescope, the worldâ€™s most advanced visible-light astronomical observatory and two survey telescopes. VISTA works in the infrared and is the worldâ€™s largest survey telescope and the VLT Survey Telescope is the largest telescope designed to exclusively survey the skies in visible light. ESO is a major partner in ALMA, the largest astronomical project in existence. And on Cerro Armazones, close to Paranal, ESO is building the 39-metre European Extremely Large Telescope, the E-ELT, which will become â€œthe worldâ€™s biggest eye on the skyâ€.
- Research paper â€“ http://www.eso.org/public/archives/releases/sciencepapers/eso1547/eso1547a.pdf
- Photos of the ESO Very Large Telescope â€“ https://www.eso.org/public/images/archive/category/paranal/
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