Galactic Social Dynamics in Protoclusters
A study reveals how galaxies interact and evolve in protoclusters.
Ian McConachie, Gillian Wilson, Ben Forrest, Z. Cemile Marsan, Adam Muzzin, M. C. Cooper, Marianna Annunziatella, Danilo Marchesini, Percy Gomez, Wenjun Chang, Stephanie M. Urbano Stawinski, Michael McDonald, Tracy Webb, Allison Noble, Brian C. Lemaux, Ekta A. Shah, Priti Staab, Lori M. Lubin, Roy R. Gal
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Table of Contents
In the vast universe, galactic conformity is like a popularity contest amongst Galaxies. You see, some galaxies prefer to hang out with their quiescent friends-those that have run out of energy and stopped forming new stars-while others are more active, constantly churning out new stars. This study dives deep into the interactions and relationships between these cosmic neighbors, especially in a fascinating region known as Protoclusters.
What Are Protoclusters?
Protoclusters are the early versions of galaxy clusters. Imagine them as the teenagers of the universe, still figuring things out, but already showing signs that they'll grow into massive, bustling clusters of galaxies as they mature. These regions are filled with many galaxies, and they can tell us a lot about how galaxies evolve over time.
Quiescent Galaxies
The Importance ofIn the cosmic world, quiescent galaxies are a bit like retired athletes. They've had their day in the sun, finishing up their Star-forming activities and settling down. Understanding them is crucial because they can reveal how galaxies change in different environments. Do they all chill out together, or do the active ones bring the quiescent ones along for the ride?
The Study's Focus
The study focuses on six protoclusters where researchers looked at the mix of star-forming and quiescent galaxies. By examining their relationships, they aim to find out if there's a pattern-like whether quiescent galaxies tend to cluster around other quiescent ones. They checked out the COSMOS field, which is a rich area in the universe that has been thoroughly mapped and observed.
The Observations
Using powerful telescopes, the researchers gathered data on over twenty galaxies in these protoclusters. They counted how many were active star-formers and how many had settled into their quiescent phase. The results were like sorting cookies: some batches turned out gooey and fresh, while others were crispy and well-baked.
The Findings
What the researchers found was quite interesting. In protoclusters with more quiescent galaxies, they also found a higher number of quiescent members in general. But in areas where the galaxies were still forming new stars, the quiescent tails were lower. It’s like having a party; if the main guest is all about relaxing, most of the partygoers seem to chill out too.
Why Does This Happen?
Researchers are scratching their heads to understand why this pattern exists. A few theories float around, like how the environment affects galaxy behaviors. It’s possible that when galaxies are born together in these dense neighborhoods, their fates become intertwined.
AGNs, or Active Galactic Nuclei, also play a role. They’re like that overly enthusiastic friend who brings energy to the party, stirring things up and influencing others. However, whether they actively help quench star formation in their surroundings is still up for debate.
The Bigger Picture
The results from this study provide a glimpse into how galaxies live, socialize, and change over time. These relationships seem to be apparent even in the early universe, about two billion years after the Big Bang. The idea that these interactions could have been in play for so long is quite revolutionary-and a little mind-bending!
Future Directions
Knowing how galaxies interact can help astronomers understand the universe better. Future studies could look at more protoclusters, examining how they change over time. Wouldn’t it be fascinating to follow these galaxies from their teenage years to their mature state, watching their relationships evolve?
Wrapping Up
In conclusion, this study sheds light on the cosmic dance of galaxies in protoclusters. It presents intriguing evidence for galactic conformity while raising plenty of questions. Just like in our own lives, the company we keep can shape who we become-whether in a cozy coffee shop or in the vastness of space.
Title: MAGAZ3NE: Evidence for Galactic Conformity in $z\gtrsim3$ Protoclusters
Abstract: We examine the quiescent fractions of massive galaxies in six $z\gtrsim3$ spectroscopically-confirmed protoclusters in the COSMOS field, one of which is newly confirmed and presented here. We report the spectroscopic confirmation of MAGAZ3NE~J100143+023021 at $z=3.122^{+0.007}_{-0.004}$ by the Massive Ancient Galaxies At $z>3$ NEar-infrared (MAGAZ3NE) survey. MAGAZ3NE~J100143+023021 contains a total of 79 protocluster members (28 spectroscopic and 51 photometric). Three spectroscopically-confirmed members are star-forming ultra-massive galaxies ($\log(M_{\star}/{\rm M}_\odot)>11$; UMGs), the most massive of which has $\log(M_{\star}/{\rm M}_\odot)=11.15^{+0.05}_{-0.06}$. Combining Keck/MOSFIRE spectroscopy and the COSMOS2020 photometric catalog, we use a weighted Gaussian kernel density estimator to map the protocluster and measure its total mass $2.25^{+1.55}_{-0.65}\times10^{14}~{\rm M}_{\odot}$ in the dense ``core'' region. For each of the six COSMOS protoclusters, we compare the quiescent fraction to the status of the central UMG as star-forming or quiescent. We observe that galaxies in these protoclusters appear to obey galactic conformity: elevated quiescent fractions are found in protoclusters with $UVJ$ quiescent UMGs and low quiescent fractions are found in protoclusters containing $UVJ$ star-forming UMGs. This correlation of star-formation/quiescence in UMGs and the massive galaxies nearby in these protoclusters is the first evidence for the existence of galactic conformity at $z>3$. Despite disagreements over mechanisms behind conformity at low redshifts, its presence at these early cosmic times would provide strong constraints on the physics proposed to drive galactic conformity.
Authors: Ian McConachie, Gillian Wilson, Ben Forrest, Z. Cemile Marsan, Adam Muzzin, M. C. Cooper, Marianna Annunziatella, Danilo Marchesini, Percy Gomez, Wenjun Chang, Stephanie M. Urbano Stawinski, Michael McDonald, Tracy Webb, Allison Noble, Brian C. Lemaux, Ekta A. Shah, Priti Staab, Lori M. Lubin, Roy R. Gal
Last Update: 2024-11-21 00:00:00
Language: English
Source URL: https://arxiv.org/abs/2411.14641
Source PDF: https://arxiv.org/pdf/2411.14641
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.
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