All images are AI generated
Quasar molecular outflow spotted by ALMA when the universe was less than a billion years old. Theoretical predictions have been confirmed with the discovery of an outflow of molecular gas from a quasar when the universe was less than a billion years old.
Quasar-Driven Molecular Outflow and Star Formation in the Early Universe
Related Video
In the vast …
Quasar Molecular Outflow: A Tale of Cosmic Evolution
A team of dedicated researchers, led by …
Quasar Molecular Outflow and Star Formation
Within galaxies, molecular gas plays a …
Quasar Molecular Outflow: Powerful Suppressor of Star Formation
The researchers sought to investigate the role …
ALMA: A Window into the Quasar Molecular Outflow
The Atacama Large Millimeter/submillimeter Array (ALMA) …
Revealing the Quasar Molecular Outflow: A Novel Approach
The researchers employed a unique technique to …
Confirmation of Theoretical Predictions: A Milestone in Understanding Quasar Molecular Outflow
The findings from this …
Quasars: Cosmic Regulators of Star Formation and Molecular Outflow
The research team concluded that …
Wrapping Up: Unraveling the Secrets of Cosmic Evolution and Quasar Molecular Outflow
This
FAQ’s
1. What are quasars, and how do they impact galaxy formation?
Quasars are immensely powerful celestial objects fueled by supermassive black holes at the centers of galaxies. Their energy output can outshine entire galaxies, and they play a significant role in galaxy formation by regulating star formation within their host galaxies.
2. How do quasars influence star formation?
Quasars can generate powerful outflows of molecular gas, which is the primary raw material for star formation. These outflows, like cosmic winds, can expel molecular gas from galaxies, effectively quenching the formation of new stars.
3. How did researchers confirm the role of quasars in suppressing star formation?
Using the Atacama Large Millimeter/submillimeter Array (ALMA), researchers employed a novel technique to detect the molecular gas outflow from a quasar-host galaxy named J2054-0005. By observing the absorption of radiation from the quasar by the outflowing gas, they confirmed the presence of the outflow and its impact on star formation.
4. What is the significance of this discovery?
This discovery provided the first concrete evidence of powerful molecular gas outflows originating from quasar-host galaxies in the early universe. It confirmed theoretical predictions and shed light on the significant role quasars play in shaping the evolution of galaxies.
5. How does this research contribute to our understanding of the early universe?
This study has opened new avenues for exploring the early universe and the role of quasars in shaping galaxy formation. By unveiling the secrets of molecular gas outflows, researchers have gained a deeper understanding of the complex interplay between quasars and their host galaxies, providing valuable insights into the intricate mechanisms that govern the evolution of the cosmos.
Links to additional Resources:
1. https://www.eso.org 2. https://www.almaobservatory.org 3. https://www.nasa.gov.Related Wikipedia Articles
Topics: Quasar (astronomy), ALMA (observatory), Atacama Large Millimeter/submillimeter Array (telescope)Quasar
A quasar ( KWAY-zar) is an extremely luminous active galactic nucleus (AGN). It is sometimes known as a quasi-stellar object, abbreviated QSO. The emission from an AGN is powered by a supermassive black hole with a mass ranging from millions to tens of billions of solar masses, surrounded by a...
Read more: Quasar
Atacama Large Millimeter Array
The Atacama Large Millimeter/submillimeter Array (ALMA) is an astronomical interferometer of 66 radio telescopes in the Atacama Desert of northern Chile, which observe electromagnetic radiation at millimeter and submillimeter wavelengths. The array has been constructed on the 5,000 m (16,000 ft) elevation Chajnantor plateau – near the Llano de Chajnantor...
Read more: Atacama Large Millimeter Array
Atacama Large Millimeter Array
The Atacama Large Millimeter/submillimeter Array (ALMA) is an astronomical interferometer of 66 radio telescopes in the Atacama Desert of northern Chile, which observe electromagnetic radiation at millimeter and submillimeter wavelengths. The array has been constructed on the 5,000 m (16,000 ft) elevation Chajnantor plateau – near the Llano de Chajnantor...
Read more: Atacama Large Millimeter Array
