To distinguish between the two options, the astronomers used both the VLTI’s Gravity instrument and the Multi Unit Spectroscopic Explorer (Muse) instrument on ESO’s VLT.ĭr Frost said: “Muse confirmed that there was no bright companion in a wider orbit, while Gravity’s high spatial resolution was able to resolve two bright sources separated by only one-third of the distance between the Earth and the Sun. “We agreed that there were two sources of light in the system, so the question was whether they orbit each other closely, as in the stripped-star scenario, or are far apart from each other, as in the black hole scenario.” Mr Rivinius said: “The scenarios we were looking for were rather clear, very different and easily distinguishable with the right instrument.
To solve the mystery, the two teams obtained new, sharper data of HR 6819 using ESO’s Very Large Telescope (VLT) and Very Large Telescope Interferometer (VLTI). “This makes our findings for HR 6819 very exciting, as it presents a perfect candidate to study how this vampirism affects the evolution of massive stars, and in turn the formation of their associated phenomena including gravitational waves and violent supernova explosions.”ĭr Frost, who led the new study published in Astronomy & Astrophysics, said: “We had reached the limit of the existing data, so we had to turn to a different observational strategy to decide between the two scenarios proposed by the two teams.” KU Leuven researcher Abigail Frost added: “Catching such a post-interaction phase is extremely difficult as it is so short. “While the donor star was stripped of some of its material, the recipient star began to spin more rapidly.” “This is a common phenomenon in close binary systems, sometimes referred to as ‘stellar vampirism’ in the press.
Referring to the new study, Dr Bodensteiner explained: “Our best interpretation so far is that we caught this binary system in a moment shortly after one of the stars had sucked the atmosphere off its companion star. This alternative scenario would mean that at an earlier stage one of the stars had stripped material from the other, sucking its essence away like a vampire. They suggested HR 6819 could also be a system with only two stars on a 40-day orbit and no black hole at all. However, a study led by Julia Bodensteiner, then a PhD student at KU Leuven, Belgium, proposed a different explanation for the same data. Thomas Rivinius, a Chile-based ESO astronomer and lead author on the original study, and his colleagues were convinced the best explanation for the data they had was that HR 6819 was a triple system, with one star orbiting a black hole every 40 days and a second star in a much wider orbit. In new research published on Tuesday, both teams united to report that there is no black hole in HR 6819, which is instead a vampire two-star system where one star has stripped material from the other. The teams agreed there were two sources of light in the system, but questions remained around whether both sources orbited each other closely – requiring one star to be stripped by the other, or were far apart – the black hole scenario.
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