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Colliding red giant prime suspect for luminous red nova outburst

Last Updated on Thursday, 09 July 2015 12:46
Published on Wednesday, 08 July 2015 23:01

Williams smallImage of a "Light Echo" illuminating dust around V838 Monocerotis (V838 Mon), another rare example of a red nova. Credit: NASA and The Hubble Heritage Team (AURA/STScI). Click for a full-size imageObservations of a rare astronomical phenomenon, called a luminous red nova, suggest that this bright outburst was caused by a red giant colliding with another star. Astronomers used the Liverpool Telescope to track the outburst over several months and hunted through the Hubble Space Telescope archive to identify possible progenitors. Dr Steven Williams will present the results at the National Astronomy Meeting 2015 in Llandudno on Thursday 9th July.

 

The outburst was first spotted in January 2015 in the Andromeda Galaxy (M31) by the Global MASTER Robotic Network, a Russian-led network of telescopes dedicated to looking for transient objects in the night sky. Williams and colleagues from Liverpool John Moores University, Dr Matt Darnley, Prof Mike Bode and Prof Iain Steele, followed the outburst with the Liverpool Telescope's new spectrometer, SPRAT, and its optical CCD camera IO:O.

 

“Initially, we thought it was a classical nova, a fairly common event. But looking at the way the brightness of the outburst evolved over time at different wavelengths, we soon realised the object in M31 was much more unusual and was a luminous red nova,” said Williams.

 

Classical novae are not particularly rare, with around 30 observed each year in M31 alone. They are thought to occur in binary systems when material falls onto the surface of a white dwarf from its larger companion star, causing a relatively short burst of nuclear fusion. By comparison, very few luminous red novae have been found to date.  Their cause is still uncertain, but the evidence suggests that they may be the result of two stars merging together, causing a very dramatic and sudden brightening of the system.

 

The LJMU team first observed the new system, dubbed M31LRN 2015, three days after its discovery. The outburst brightened over several days. After reaching a peak, optical observations showed the luminous red nova fading quickly in bluer wavelengths, but remaining bright in the redder wavelengths for several weeks.  Spectral analysis of the light showed an initial burst of hydrogen emission. As this faded, spectral features resembling a cool red star emerged. The outburst was observed again in May, and had all but disappeared in the optical, but was still bright at infrared wavelengths.

 

The team used an image of the outburst taken with the Liverpool Telescope to determine precisely the position of the system. Next, they searched the Hubble Space Telescope data archives for objects in the same place. An image taken in 2004 showed the likely progenitor star: a red giant.

 

Interestingly, the system appears to show evidence of hydrogen emission many years prior to the outburst, although the source of this emission is not clear.

 

“We found that our observations of M31LRN 2015 showed strong similarities to other objects classified as luminous red novae. If a single mechanism is responsible for all these rare events, the evidence suggests merging stars as the cause,” said Williams. He added, “Further observations of this and other systems are certainly needed. Astronomers have some way to go before these enigmatic objects are fully understood.”

 


Media contacts

 

Dr Robert Massey

Royal Astronomical Society

Mob: +44 (0)794 124 8035

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Ms Anita Heward

Royal Astronomical Society

Mob: +44 (0)7756 034 243

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Dr Sam Lindsay

Royal Astronomical Society

Mob: +44 (0)7957 566 861

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Science contacts

 

Dr Steven Williams

Astrophysics Research Institute

Liverpool John Moores University

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www.astro.ljmu.ac.uk/~scw

 


Further information

 

"A Luminous Red Nova in M31 and its Progenitor System", The Astrophysical Journal Letters, Volume 805, Issue 2, article id. L18, 6 pp. (2015).

 


Notes for editors

 

The Royal Astronomical Society National Astronomy Meeting (NAM 2015) will take place in Llandudno, Wales, from 5-9 July. NAM 2015 will be held in conjunction with the annual meetings of the UK Solar Physics (UKSP) and Magnetosphere Ionosphere Solar-Terrestrial physics (MIST) groups. The conference is principally sponsored by the Royal Astronomical Society (RAS) and the Science and Technology Facilities Council (STFC). Follow the conference on Twitter

 

The Royal Astronomical Society (RAS), founded in 1820, encourages and promotes the study of astronomy, solar-system science, geophysics and closely related branches of science. The RAS organises scientific meetings, publishes international research and review journals, recognises outstanding achievements by the award of medals and prizes, maintains an extensive library, supports education through grants and outreach activities and represents UK astronomy nationally and internationally. Its more than 3800 members (Fellows), a third based overseas, include scientific researchers in universities, observatories and laboratories as well as historians of astronomy and others. Follow the RAS on Twitter

 

The Science and Technology Facilities Council (STFC) is keeping the UK at the forefront of international science and tackling some of the most significant challenges facing society such as meeting our future energy needs, monitoring and understanding climate change, and global security. The Council has a broad science portfolio and works with the academic and industrial communities to share its expertise in materials science, space and ground-based astronomy technologies, laser science, microelectronics, wafer scale manufacturing, particle and nuclear physics, alternative energy production, radio communications and radar. It enables UK researchers to access leading international science facilities for example in the area of astronomy, the European Southern Observatory. Follow STFC on Twitter