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New research using NASA’s Stratospheric Observatory for Infrared Astronomy (SOFIA) suggests that the formation of stars can be regulated by stellar winds, shedding new light on how stars are born.

Previously, it was believed that cosmic processes such as supernovae were responsible for regulating the way in which new stars formed. Now according to the new research, it seems that the stellar winds that are generated when a star is born may prevent new stars from forming nearby. Stellar winds are fast moving flows of material that are ejected outwards from a star, and this new data shows that they can blow away the materials that are required to create new stars, preventing stars from being born too close to other newborn stars in a process called feedback.

The findings come from observations of the Orion Nebula, one of the most photographed objects in the night sky and the closest stellar nursery to Earth. Using infrared light, scientists are able to peer through the clouds of dust and gas shrouding the nebula to observe the process of star birth happening within. They saw that a baby star called Theta1 Orionis C (θ1 Ori C) was generating strong stellar winds which were sweeping up large amounts of material from the cloud around the star, “like a snow plow clearing a street by pushing snow to the road’s edges.”

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The powerful wind from the newly formed star at the heart of the Orion Nebula is creating the bubble (black) and preventing new stars from forming in its neighborhood. At the same time, the wind pushes molecular gas (color) to the edges, creating a dense shell around the bubble where future generations of stars can form. NASA/SOFIA/Pabst et al.

“The wind is responsible for blowing an enormous bubble around the central stars,” lead author Cornelia Pabst, Ph.D. student at the University of Leiden, the Netherlands, said in a statement. “It disrupts the natal cloud and prevents the birth of new stars.”

SOFIA is a flying observatory in a modified Boeing 747SP jetliner aircraft which can fly above 99 percent of the water vapor in Earth’s atmosphere, allowing instruments like the German Receiver for Astronomy at Terahertz Frequencies (GREAT) to detect infrared light that would otherwise be blocked by the vapor. The GREAT instrument measured the spectral signature of ionized carbon to determine the speed of gas moving in the distant nebula “like a police officer uses a radar gun,” according to co-author Alexander Tielens.

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NASA’s SOFIA airborne observatory is shadowed by a NASA F/A-18 safety chase aircraft during its second checkout flight near Waco, Texas on May 10, 2007. NASA

The findings are published in Nature.








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