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The Intriguing World of Galaxies

Explore the diverse shapes and formations of galaxies throughout the universe.

Sungwook E. Hong, Changbom Park, Preetish K. Mishra, Juhan Kim, Brad K. Gibson, Yonghwi Kim, C. Gareth Few, Christophe Pichon, Jihye Shin, Jaehyun Lee

― 6 min read


Galaxies: Shapes and Galaxies: Shapes and Stars galaxies and their star formation. Investigate the dynamic nature of
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Have you ever looked up at the night sky and wondered about the stars and the worlds they belong to? Galaxies are like enormous neighborhoods in space, filled with stars, dust, and gas. They come in different shapes and sizes, just like people. Some are round and puffy, while others are flat and spiral-shaped. What makes these galaxies look different? And how do they form stars? Let's dive into this fascinating topic without getting lost in complex science words.

What Are Galaxies?

Galaxies are vast collections of stars, planets, gas, and dust held together by gravity. Imagine a massive city filled with millions of people, but instead of buildings, there are stars and planets. Our home, the Milky Way, is just one of the billions of galaxies in the universe.

There are three main types of galaxies:

  1. Spiral Galaxies: These look like giant pinwheels, with arms winding out from a central bulge. The Milky Way is one of these.

  2. Elliptical Galaxies: These are smooth and rounded, looking like a giant puffed-up ball. They don’t have the spiral arms and are typically home to older stars.

  3. Irregular Galaxies: These don't fit nicely into the other categories. They are messy and chaotic, often lacking a defined shape.

The Shapes of Galaxies

The shapes of galaxies tell astronomers a lot about their lives. Spiral galaxies, with their pretty arms, are often full of young stars, while elliptical galaxies, which look a bit like swollen marshmallows, are mostly made up of older stars. Irregular galaxies make for an exciting mix, swarming with star-forming activity in a cosmic dance.

Why Do Galaxies Have Different Shapes?

The shape of a galaxy can be thought of like the history of a person. Each galaxy goes through different life events that shape who they are. For example, when galaxies collide or merge, they can change shape dramatically. This is similar to how people’s personalities can change after significant life events, like moving to a new city or starting a new job.

Stars and Star Formation

Stars are like the bright lights in a galaxy's sky. They are born from clouds of gas and dust collapsing under gravity's pull. This is the beginning of a star’s life cycle, and it’s a process that can take millions of years-kind of like waiting for your favorite pizza to come out of the oven!

The Life of a Star

Once a star is born, it goes through several stages:

  1. Main Sequence: This is the longest phase, where the star shines steadily, like a lamp on a timer.

  2. Red Giant: As the star runs out of fuel, it swells up, becoming bigger and redder. Think of it as a balloon that keeps getting bigger but is about to pop!

  3. Supernova: If the star is massive enough, it may explode in a brilliant burst of light, called a supernova. This is like the grand finale of a fireworks show!

  4. Black Hole or Neutron Star: After the explosion, the remnants can form a dense neutron star or even collapse into a black hole, which is a region in space where gravity is so strong that nothing, not even light, can escape.

Galaxy Clusters

Galaxies don’t float around in isolation; they often gather together in groups known as galaxy clusters. Think of these clusters as the bustling neighborhoods of the universe. In these clusters, galaxies can interact with one another, leading to changes in their shapes and star production.

How Are Cluster Galaxies Different?

Galaxies in clusters have different characteristics compared to those in isolation. They might be more influenced by their neighbors, leading to changes in their shape and star formation activity. You could say that living in a crowded area pushes them to meet new friends and evolve!

The Connection Between Shape and Star Formation

One of the intriguing questions in astronomy is how the shape of a galaxy affects its ability to create new stars. Spiral galaxies, with their abundant gas and dust, are often star-making factories. In contrast, elliptical galaxies have fewer star-forming materials left, making them more like quiet retirement communities for older stars.

Galaxies in Different Environments

The location of a galaxy matters, too. Those in dense clusters tend to be different from those in the vast emptiness of space. In clusters, galaxies can experience interactions that can squish their shapes or trigger bursts of star formation. It’s like being at a party where some people are social butterflies while others prefer to sit quietly in the corner.

Studying Galaxy Morphology

Astronomers study the shapes of galaxies to understand their histories better. By looking at their morphology, or shape, scientists can figure out how galaxies have interacted over time, how many stars they host, and what types of stars they are forming.

Tools for Observing Galaxies

With advanced telescopes, astronomers gather images of galaxies and analyze them. By examining their light, scientists can learn about a galaxy's composition, temperature, density, and motion. It's a bit like a detective gathering clues to solve a mystery!

The Role of Simulations

One way that researchers study galaxies is by using simulations-these are computer models that mimic galaxy formation and evolution. Just like a video game allows players to explore different scenarios, simulations let astronomers test their ideas about how galaxies change over time.

What Do Simulations Show Us?

Simulations can reveal how galaxies merge, how star formation happens, and how different environments affect galaxy shapes. They provide a valuable playground for understanding the complex processes that shape our universe.

The Importance of Cosmic Time

The universe is constantly changing, and so are galaxies. Cosmic time refers to the timeline of the universe's evolution. As the universe ages, galaxies evolve too. It's essential to consider this timeline when discussing galaxy shapes and star formation.

What Happens Over Time?

As galaxies age, they might change from spiral shapes to more rounded forms. This transformation can be driven by several factors, including interactions with other galaxies and the availability of gas for star formation. Over billions of years, the environment plays a significant role in these developments.

Conclusion

Galaxies are not just distant specks of light; they are complex and dynamic systems shaped by their histories. Understanding the relationship between a galaxy's shape and its star formation can help us piece together the cosmic puzzle of how our universe develops. So next time you gaze up at the night sky, remember that each twinkling star belongs to a galaxy with its own unique story, shaped by time and space-a story that keeps unfolding as the universe continues to evolve.

Original Source

Title: Emergence of the Galaxy Morphology-Star Formation Activity-Clustercentric Radius Relations in Galaxy Clusters

Abstract: We investigate when and how the relations of galaxy morphology and star forming activity with clustercentric radius become evident in galaxy clusters. We identify 162 galaxy clusters with total mass $M_{\rm tot}^{\rm cl} > 5 \times 10^{13} {\rm M}_\odot$ at $z = 0.625$ in the Horizon Run 5 (HR5) cosmological hydrodynamical simulation and study how the properties of the galaxies with stellar mass $M_\ast > 5 \times 10^9 {\rm M}_\odot$ near the cluster main progenitors have evolved in the past. Galaxies are classified into disk, spheroid, and irregular morphological types according to the asymmetry and Sersic index of their stellar mass distribution. We also classify galaxies into active and passive ones depending on their specific star-formation rate. We find that the morphology-clustercentric radius relation (MRR) emerges at $z \simeq 1.8$ as the fraction of spheroidal types exceeds 50% in the central region ($d \lesssim 0.1 R_{200}$). Galaxies outside the central region remain disk-dominated. Numerous encounters between galaxies in the central region seem to be responsible for the morphology transformation from disks to spheroids. We also find that the star formation activity-clustercentric radius relation emerges at an epoch different from that of MRR. At $z\simeq0.8$, passive galaxies start to dominate the intermediate radius region ($0.1\lesssim d/R_{200} \lesssim0.3$) and this "quenching region" grows inward and outward thereafter. The region dominated by early-type galaxies (spheroids and passive disks) first appears at the central region at $z\simeq 1.8$, expands rapidly to larger radii as the population of passive disks grows in the intermediate radii, and clusters are dominated by early types after $z\simeq 0.8$.

Authors: Sungwook E. Hong, Changbom Park, Preetish K. Mishra, Juhan Kim, Brad K. Gibson, Yonghwi Kim, C. Gareth Few, Christophe Pichon, Jihye Shin, Jaehyun Lee

Last Update: 2024-11-12 00:00:00

Language: English

Source URL: https://arxiv.org/abs/2411.08255

Source PDF: https://arxiv.org/pdf/2411.08255

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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