Ultra-close stars discovered inside a planetary nebula
The newly discovered binary system in the centre of the planetary nebula M3-1 has one of the shortest orbital periods ever seen inside such an object. The findings of the study, published in MNRAS Letters, reveal that the interaction between the two stars could quickly lead to a nova explosion, something which is not predicted by theories of binary evolution.
An international team of astronomers, led by David Jones from the Instituto de Astrofísica de Canarias (IAC) and Universidad de La Laguna (ULL), with significant participation by Paulina Sowicka, PhD student at the Nicolaus Copernicus Astronomical Centre in Warsaw, Poland, have discovered a binary system with an orbital period of just a little over three hours. The discovery, which involved several years of observing campaigns, is not only surprising due to the extremely short orbital period but also in that, due to their close proximity to one another, the system may result in a nova explosion before the short-lived nebula has dissipated. The results of the study were published in the prestigious scientific journal Monthly Notices of the Royal Astronomical Society (MNRAS).
Planetary nebulae are the glowing shells of gas and dust ejected from Sun-like stars towards the ends of their lives. "In many cases, we see that the ejection is driven by the interaction between the progenitor star and a close companion, and this is leads to the vast array of elaborate shapes and structures we see in the nebulae", explains Jones. The study focused on the planetary nebula M3-1, a firm candidate to have been the product of a binary system due to its spectacular jets, which are typically formed by the interaction of two stars. According to Brent Miszalski, researcher at the SALT telescope in South Africa and co-author of the work, "We knew it had to contain a binary, that's why we decided to study the system to try and understand the relationship between the stars and the nebula they have formed".
The observations quickly confirmed the researchers suspicions. "When we began observing it was immediately clear that it was, indeed, a binary. Moreover, the brightness of the system was changing very quickly and this could mean a rather short orbital period", says Henri Boffin, researcher at the European Southern Observatory (ESO) in Germany. In fact, the study revealed the separation between the stars to be, approximately, 160,000 kilometres, or less than half the distance between the Moon and the Earth.
After various observing campaigns in Chile with ESO's Very Large Telescope (VLT) and New Technology Telescope (NTT), the researchers had enough data to work out the properties of the binary system, like the masses, temperatures and sizes of both stars. "To our surprise, we discovered that the two stars were quite big and that, as they are so close to one another, it is very likely that they will begin to interact again in just another few thousand years perhaps resulting in nova explosion" adds Paulina Sowicka, PhD student at the Nicolaus Copernicus Astronomical Centre in Warsaw, Poland.
The result contradicts current theories of binary stellar evolution which predict that, upon forming the planetary nebula, the two stars should take quite a long time before beginning to interact again. By the time they do, the nebula should have dispersed and should no longer be visible. However, a nova explosion in 2007, known as Nova Vul 2007, was found to be inside another planetary nebula, putting into question the models. In the case of M3-1, a candidate to experience a similar evolution has now been found. Given that the stars are almost touching, they should (on astronomical time scales) soon interact again and, perhaps, producing another nova inside a planetary nebula.
Article: Jones, D. et al. The short orbital period binary star at the heart of the planetary nebula M 3-1. Monthly Notices of the Royal Astronomical Society: Letters, 482, L75, https://doi.org/10.1093/mnrasl/sly142.
Source: CAMK PAN
