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Webb Marks Third Anniversary With Infrared Views of Star-Forming Cores in Cat’s Paw Nebula

The findings illuminate the role of stellar feedback in shaping gas and dust within active stellar nurseries.

La nebulosa Pata de Gato se vuelve así un laboratorio natural para comprender el ciclo de vida de las estrellas y, en última instancia, el origen de sistemas como el nuestro.
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Overview

  • Webb’s NIRCam instrument pierced dense dust in NGC 6334 to reveal mini “pads” containing young massive stars sculpting their surroundings.
  • The observations demonstrate how energetic radiation and stellar winds carve cavities in gas and dust and eventually halt local star birth.
  • Situated about 4,000 light-years away in Scorpius, the Cat’s Paw Nebula ranks among the Milky Way’s most active stellar nurseries and rewards infrared inspection.
  • These images deliver resolution far beyond prior Hubble and Spitzer data, underscoring Webb’s success in uncovering previously hidden cosmic processes.
  • Insights from these latest observations are shaping science goals for forthcoming flagship missions such as the Nancy Grace Roman Telescope and the Habitable Worlds Observatory.