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Massive stars may not be as “giant” as previously thought

Research on the core of the Tarantula Nebula or 30 Doradus nebula appeared in the latest edition of the Astrophysical Journal.

What was previously believed to be a massive star located in the center of the Tarantula Nebula, also known as 30 Doradus, is actually a cluster of stars, as discovered by recent research analyzing the star R136. R136 is one of the stars forming the Large Magellanic Cloud, a region that harbors the most massive stars ever found. These stars’ brightness is so intense that they can be viewed with the naked eye.

The research, published in the latest edition of the Astrophysical Journal, involved Dr. Mónica Rubio, winner of the 2021 National Exact Sciences Award and astronomer at the University of Chile who is part of the Center for Astrophysics and Related Technologies, CATA. “The highest mass stars are not as massive as we thought,” explains Rubio, regarding the new study, which could make us rethink the models of star formation and its final stages.

Dr. Rubio adds that getting these results required more than a year of research using the Gemini South Telescope, located in Cerro Pachón in the Coquimbo Region, in which Chile participates through the observation time for national astronomers administered by the National Agency for Research and Development, ANID. “It was the large 8.1m mirror and the instrument called “Zorro” that allowed us to take the sharpest optical images that can be taken from the ground today, revealing that where we thought there was only one star, there are actually several.

Rubio also explains that the next step will be to continue with this research and determine the properties of these stars, since they are not as massive as previously thought, “it could imply that perhaps the first stars in the universe were not as massive as the models require”, says the astronomer. “This can be elucidated with future observations only possible with the James Webb Telescope,” she adds.

Also participating in this work were Venu Kalari, who is the lead author of the paper, and Ricardo Salinas, an astronomer at the Gemini South observatory in the Coquimbo Region, in addition to the collaboration of Chilean engineers from the observatory, together with a team from NASA. The results were published under the title “Resolving the core of R136 in the optical”, published in the latest edition of the Astrophysical Journal.