Research news on Star forming regions

Star forming regions as a research area focuses on the physical processes governing the collapse of molecular clouds and the subsequent birth of stars and planetary systems. This field investigates the interplay of gravity, turbulence, magnetic fields, and feedback from young stellar objects using multiwavelength observations (radio to X-ray) and magnetohydrodynamic simulations. Key topics include the initial mass function, core and filament formation, protostellar accretion, disk evolution, and triggered versus spontaneous star formation. Research also addresses chemical evolution in dense cores, the role of environment (e.g., metallicity, radiation fields), and the impact of stellar feedback on regulating star formation efficiency and shaping galactic structure.

Webb image reveals young stars brewing in a nebulous cauldron

In this Picture of the Month from the NASA/ESA James Webb Space Telescope, we visit a turbulent cauldron of star formation to see what is brewing inside dense clumps of gas. This is a star-forming region named LHA 120-N 159, ...

Webb captures commotion from nebula's stellar jets

The NASA/ESA/CSA James Webb Space Telescope has unveiled numerous stars formerly hidden by clouds of dust in a stellar nursery known as NGC 7129—a cauldron of cosmic creation, 3,300 light-years from Earth. Webb captured infrared ...

Turbulent times for star formation in Stephan's Quintet

Star formation in galaxies is closely linked to molecular gas. In the distant past, when galaxy interactions were more common, these encounters compressed molecular gas, causing dense clouds to collapse under their own gravity ...

Photo: NASA's Hubble spies superbubble scene

This NASA/ESA Hubble Space Telescope image features a sprawling cosmic vista in the Large Magellanic Cloud, or LMC, the largest of the small galaxies that orbit our Milky Way galaxy. At just 160,000 light-years away, the ...

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