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The Interplay of Stars and Black Holes in Galaxies

Exploring how stars and black holes influence each other in the universe.

Leah K. Morabito, R. Kondapally, P. N. Best, B. -H. Yue, J. M. G. H. J. de Jong, F. Sweijen, Marco Bondi, Dominik J. Schwarz, D. J. B. Smith, R. J. van Weeren, H. J. A. Röttgering, T. W. Shimwell, Isabella Prandoni

― 6 min read


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In the vast universe, Galaxies twirl and spin, much like dancers in a cosmic ballet. At the heart of many of these galaxies lies a super-massive black hole, which is like a huge vacuum cleaner that gobbles up whatever comes too close. Meanwhile, stars within these galaxies are busy forming, shining, and living their own lives. This interaction between stars and Black Holes-let's call it a “power couple” scenario-has scientists scratching their heads. They want to know how these two forces impact each other over time.

To figure this out, astronomers take a closer look at galaxies, especially at how stars are born and how black holes grow. They’ve come up with a clever way to measure the brightness of Radio Waves emitted from galaxies. Think of radio waves as the gossip of the galaxy, revealing secrets about Star Formation and black hole activity. By looking at this radio “gossip,” researchers can figure out who is doing what in the galaxy.

The Role of Radio Waves

Imagine if you could listen in on a conversation and get clues about who is the loudest and who is quietly lurking in the background. This is what radio waves allow scientists to do. They can tell if a galaxy is bustling with star formation or if it’s a black hole party.

Now, to collect this radio gossip, astronomers use advanced telescopes that are like the super-sleuths of space. One such telescope is the International LOFAR Telescope, which operates at a lower frequency that lets it hear distant and faint radio waves. With LOFAR, astronomers can distinguish between the sounds of stars forming and the whispers of black holes efficiently.

Star Formation vs. Black Holes: A Delicate Balance

In this cosmic drama, both star formation and black hole activity are key players. When a galaxy is forming stars, it can be joyful and vibrant. However, at the same time, if the black hole is active, it can overshadow the star formation. Sometimes, black holes emit jets of energy that can hinder star growth. It’s like having a party where one guest (the black hole) is so loud that no one else can enjoy themselves.

In the past, astronomers would label galaxies simply as star-forming or black hole-dominated based on how they appeared. But this wasn’t accurate. Mixing them up could mean that some black holes got too much credit while star formation was slighted, or vice versa.

Breaking It Down

To address this mix-up, researchers decided to roll up their sleeves and get to work. By combining images from LOFAR, they could identify the parts of galaxies that were producing radio waves from stars and those that were being affected by black holes.

They took a closer look at two regions in the sky, called the Lockman Hole and the ELAIS-N1 fields, which are like two cosmic neighborhoods. The scientists scrutinized nearly 7,500 galaxies in this area, measuring the Brightness Temperature of the radio waves to separate the contributions from stars and black holes.

The Hidden Black Hole Population

What happened was rather surprising. As they took away the contributions from the black holes, they uncovered a hidden population of black holes that had been misclassified as just “star-forming.” It’s like finding out that a quiet person at a party is actually a famous celebrity-they were there all along, just not getting any attention.

When they crunched the numbers, they found that there were 1.56 times more black holes than they had expected when looking at galaxies in the old way. Meanwhile, the expected star-forming population was only 0.90 times as present as anticipated. This had huge implications for how they calculate the cosmic star formation rate and other metrics.

Observing the Cosmic Clock

So, as scientists study the cosmos further, they are trying to understand how black holes and star formation evolve over time. To do this, they break their observations into slices of time called “redshift bins.” Each bin represents a different period in the universe's history.

During these observations, researchers noted how both star formation and black hole activity changed over time. It was like watching the style changes of music through the decades. They found that while star formation had a clear trend, black hole activity seemed to be more stable, not going through drastic changes.

The Magic of LOFAR

The success of this study hinged on the unique capabilities of LOFAR. It offers high resolution, which is crucial for distinguishing between the two players in this cosmic game. LOFAR’s wide field of view is like having zoomed-in binoculars, allowing astronomers to spot many galaxies at once without losing detail.

This kind of detailed imaging means researchers can gather a ton of data quickly. In fact, they managed to get images of 2,483 sources in Lockman Hole and 13,058 sources in ELAIS-N1. This massive dataset is a giant leap forward for understanding the universe.

The Brightness Temperature Trick

One of the ingenious tactics used in this research was measuring what’s called brightness temperature. While it sounds complicated, it’s merely a way to gauge how bright a galaxy is from radio emissions. If a galaxy is too bright according to predictions from star formation models, then astronomers tag it as being influenced by a black hole.

This is a game-changer because it allows precise identification of black hole components in galaxies. Using this method creates a clearer picture of how black holes are affecting star formation.

Looking Forward

With this new knowledge, scientists are gearing up to refine their methods and explore the complexities of cosmic communities further. They want to clarify how often galaxies have these hidden black holes and how this impacts our understanding of the universe’s energy output.

Future research will also look at how other elements of the universe interact. This could pave the way for connecting observations of galaxies with computer simulations that model the universe’s structure.

Why Does This Matter?

Why should anyone care about black holes and stars? Well, the relationships between these cosmic entities affect how galaxies evolve. Understanding these dynamics helps scientists piece together the history of the universe itself.

Additionally, with the newfound knowledge about hidden black holes and their role in galaxies, theories about the cosmic star formation rate could shift. This information might change how researchers view the energy landscape of the universe, which can impact everything from the formation of new stars to the lifecycle of galaxies.

Conclusion: The Cosmic Harmony

In essence, this exploration of galaxies brings us closer to understanding the cosmic choir-a harmonious blend of star formation and black hole activity. Just like in an orchestra, where different instruments create a beautiful symphony together, galaxies need both stars and black holes to evolve gracefully.

As researchers continue to peel back the layers of the cosmos using advanced tools like LOFAR, it’s likely that more secrets will be uncovered. We might find more surprises hiding in the shadows, all waiting patiently for their moment in the spotlight. So grab your telescope, and let’s keep gazing at the stars; who knows what we’ll find next in this vast and mysterious universe!

Original Source

Title: A hidden Active Galactic Nuclei population: the first radio luminosity functions constructed by physical process

Abstract: Both star formation (SF) and Active Galactic Nuclei (AGN) play an important role in galaxy evolution. Statistically quantifying their relative importance can be done using radio luminosity functions. Until now these relied on galaxy classifications, where sources with a mixture of radio emission from SF and AGN are labelled as either a star-forming galaxy or an AGN. This can cause the misestimation of the relevance of AGN. Brightness temperature measurements at 144 MHz with the International LOFAR telescope can separate radio emission from AGN and SF. We use the combination of sub-arcsec and arcsec resolution imaging of 7,497 sources in the Lockman Hole and ELAIS-N1 fields to identify AGN components in the sub-arcsec resolution images and subtract them from the total flux density, leaving flux density from SF only. We construct, for the first time, radio luminosity functions by physical process, either SF or AGN activity, revealing a hidden AGN population at $L_{\textrm{144MHz}}$$

Authors: Leah K. Morabito, R. Kondapally, P. N. Best, B. -H. Yue, J. M. G. H. J. de Jong, F. Sweijen, Marco Bondi, Dominik J. Schwarz, D. J. B. Smith, R. J. van Weeren, H. J. A. Röttgering, T. W. Shimwell, Isabella Prandoni

Last Update: 2024-11-07 00:00:00

Language: English

Source URL: https://arxiv.org/abs/2411.05069

Source PDF: https://arxiv.org/pdf/2411.05069

Licence: https://creativecommons.org/licenses/by/4.0/

Changes: This summary was created with assistance from AI and may have inaccuracies. For accurate information, please refer to the original source documents linked here.

Thank you to arxiv for use of its open access interoperability.

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