Young massive stars in the central parsec of our Galaxy are best explained by star formation within at least one, and possibly two, massive self-gravitating gaseous discs. With help of numerical ...

Radiation transport plays a crucial role in star formation models, as certain questions within this field cannot be accurately addressed without taking it into account. Given the high complexity of ...

Previous observations provided tantalizing hints of a young massive planet orbiting this star very close,” study co-author Sergei Nayakshin said. “We discovered a new process which you might ...

Planet demise ends the outburst. Credit: Sergei Nayakshin/Vardan Elbakyan, University of Leicester They have published their findings in the journal Monthly Notices of the Royal Astronomical Society.

ABSTRACT: Magnetic field can be amplified and twisted near a supermassive black hole residing in a galactic nucleus. At the same time magnetic null points develop near the horizon. We examine a ...

"We discovered a new process which you might call a 'disc inferno' of young planets," University of Leicester School of Physics and Astronomy professor Sergei Nayakshin said in a statement.

We discovered a new process which you might call a ‘disc inferno’ of young planets,” lead author Professor Sergei Nayakshin from the University of Leicester said in a statement. The ...

Lead author Professor Sergei Nayakshin from the University of Leicester School of Physics and Astronomy said, "These disks feed growing stars with more material but also nurture planets.