© ESO/M. KornmesserUsing a combination of instruments on ESO's Very Large Telescope, astronomers have discovered the most massive stars to date, some weighing at birth more than 300 times the mass of the Sun, or twice as much as the currently accepted limit of 150 solar masses. This artist's impression shows the relative sizes of young stars, from the smallest "red dwarfs", weighing in at about 0.1 solar masses, through low mass "yellow dwarfs" such as the Sun, to massive "blue dwarf" stars weighing eight times more than the Sun, as well as the 300 solar mass star named R136a1.
Using a combination of instruments on ESO's Very Large Telescope, a UK-led international team of astronomers have discovered the most massive stars to date, one which at birth had more than 300 times the mass of the Sun, twice as much as the currently accepted limit.
The existence of these monsters - millions of times more luminous than the Sun, losing mass through very powerful winds - may provide an answer to the question "how massive can stars be?" The new results appear in a paper in the journal
Monthly Notices of the Royal Astronomical Society.
A team of astronomers led by Paul Crowther, Professor of Astrophysics at the University of Sheffield, used ESO's Very Large Telescope, as well as archival data from the NASA/ESA Hubble Space Telescope, to study two young clusters of stars, NGC 3603 and RMC 136a in detail. NGC 3603 is a cosmic factory where stars form frantically from the nebula's extended clouds of gas and dust, located 22,000 light-years away from the Sun (eso1005).
RMC 136a (more often nicknamed R136) is another cluster of young, massive and hot stars, which is located inside the Tarantula Nebula, in one of our neighboring galaxies, the Large Magellanic Cloud, 165,000 light-years away (eso0613).