The universe's supermassive black holes have been growing in a previously unknown way, scientists say. Researchers propose that these behemoths of gravity are surrounded by high-density gas cocoons during their early stages of development.
This cocoon phase is believed to be the reason why young supermassive black holes appear much more massive than expected when observing them through infrared light. The cosmic shield created by this dense material absorbs X-rays and radio waves, making these objects difficult to detect using standard telescopes like Chandra.
According to a new study published in Nature, scientists observed 12 Little Red Dots - galaxies that are believed to host supermassive black holes of unprecedented mass. By applying a scattering model to the data from these galaxies, researchers found that the intrinsic velocity of the gas surrounding these young black holes is much lower than previously thought.
The cocoon phase model suggests that these young black holes grow rapidly, surrounded by a dense shell of gas and dust. This cosmic shield blocks high-energy radiation, explaining why these objects are so bright in infrared light but virtually invisible to X-ray telescopes.
While the study provides an elegant solution to the mass problem, questions remain about how long this cocoon phase lasts and how common it is in the early universe. Further analysis of new high-resolution data from the James Webb Space Telescope may shed more light on these mysteries.
The implications of this discovery are significant, as it challenges our current understanding of galaxy formation and the role of supermassive black holes in their development.
This cocoon phase is believed to be the reason why young supermassive black holes appear much more massive than expected when observing them through infrared light. The cosmic shield created by this dense material absorbs X-rays and radio waves, making these objects difficult to detect using standard telescopes like Chandra.
According to a new study published in Nature, scientists observed 12 Little Red Dots - galaxies that are believed to host supermassive black holes of unprecedented mass. By applying a scattering model to the data from these galaxies, researchers found that the intrinsic velocity of the gas surrounding these young black holes is much lower than previously thought.
The cocoon phase model suggests that these young black holes grow rapidly, surrounded by a dense shell of gas and dust. This cosmic shield blocks high-energy radiation, explaining why these objects are so bright in infrared light but virtually invisible to X-ray telescopes.
While the study provides an elegant solution to the mass problem, questions remain about how long this cocoon phase lasts and how common it is in the early universe. Further analysis of new high-resolution data from the James Webb Space Telescope may shed more light on these mysteries.
The implications of this discovery are significant, as it challenges our current understanding of galaxy formation and the role of supermassive black holes in their development.