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# Physics# Astrophysics of Galaxies

Bright Changes in Distant Quasars

Recent discoveries reveal dynamic behaviors of changing-look quasars across the universe.

Wei-Jian Guo, Zhiwei Pan, Małgorzata Siudek, Jessica Nicole Aguilar, Steven Ahlen, Davide Bianchi, David Brooks, Todd Claybaugh, Kyle Dawson, Axel de la Macorra, Peter Doel, Kevin Fanning, Jaime E. Forero-Romero, Enrique Gaztañaga, Satya Gontcho A Gontcho, Klaus Honscheid, Robert Kehoe, Theodore Kisner, Andrew Lambert, Martin Landriau, Laurent Le Guillou, Marc Manera, Aaron Meisner, John Moustakas, Andrea Muñoz-Gutiérrez, Adam Myers, Jundan Nie, Nathalie Palanque-Delabrouille, Claire Poppett, Francisco Prada, Mehdi Rezaie, Graziano Rossi, Eusebio Sanchez, Michael Schubnelll, Hee-Jong Seo, Joseph Harry Silber, David Sprayberry, Gregory Tarlé, Benjamin Alan Weaver, Zhimin Zhou, Hu Zou

― 6 min read


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Table of Contents

Quasars are some of the brightest objects in the universe. They are powered by Supermassive Black Holes at the center of galaxies. Sometimes, these quasars show changes in their brightness and the types of light they emit. These changes are called "changing-look" events. In this article, we will discuss a few quasars that have displayed this behavior and what it means for our understanding of space.

What Are Quasars?

Quasars are incredibly bright and faraway objects. They are actually a type of galaxy with an active black hole. The material falling into the black hole heats up, emitting lots of light. Think of them as cosmic lighthouses, shining brightly across vast distances. Some quasars are so bright that we can see them even when they are billions of light-years away.

Changing-Look Quasars

Changing-look quasars are those that change their appearance over time. This can mean a shift in brightness or even changes in the light spectrum they emit. This phenomenon can happen quite rapidly, sometimes within a few months or years. It's like a chameleon that decides to change its color but on a cosmic scale!

A New Discovery

Recently, astronomers discovered four new quasars that exhibit this changing behavior. The names of these quasars are J1306, J1512, J1511, and J1602. What’s special about these findings is that they represent the first time researchers could observe these changes in a specific type of light called Ly (Lyman-alpha) at a great distance in space. This is kind of a big deal in the astronomy community, like finding the last piece of a jigsaw puzzle after years of searching.

How They're Found

These quasars were spotted using two major observational projects: the Dark Energy Spectroscopic Instrument (DESI) and the Sloan Digital Sky Survey (SDSS). Both of these initiatives are designed to find and study distant objects in space. It’s like using a super-powered magnifying glass to inspect the universe's faintest features.

Change is Confirmed!

What gives scientists confidence that these quasars really are changing? It's the noticeable differences in brightness and the light they emit. For J1306 and J1512, the researchers saw a significant difference in the brightness of the Ly light. In simpler terms, if you imagine turning the lights on and off in a room, these quasars are doing just that-brightening and dimming in a cosmic dance.

Black Holes at the Core

So, what causes these changes? The heart of each quasar is a supermassive black hole. As material falls into these black holes, it can lead to variations in light output. If the black hole gets a hearty meal, it can shine brightly. If its "dinner" slows down, so does its brightness. The study of these changes helps scientists understand how black holes consume material and interact with their surroundings.

The Accretion Disk

Around each black hole is a disk of gas and dust known as the accretion disk. This is where the action happens. It’s similar to a whirlpool, where material spins around before falling in. The state of this disk can change, leading to the quasar’s changing appearance. Sometimes, the disk may switch from a more chaotic state to a calmer one, affecting how bright the quasar seems.

The Role of Light

Different types of light can offer clues about what’s happening inside these quasars. Light from the Ly spectrum is particularly important because it comes from the innermost regions of the accretion disk. It can even show us how fast the material is moving. Variations in this light can tell scientists a lot about changes happening at the center of the quasar.

What About the Candidates?

In addition to the already mentioned J1306 and J1512, the researchers identified two more candidates that may also undergo changing-look events: J1511 and J1602. While they haven’t been confirmed yet, they show signs that they might belong in the same club of changing-look quasars. It’s like finding potential members for an exclusive cosmic club!

How Do We Measure Changes?

To figure out if these quasars are really changing, researchers analyze the light they emit. They look for changes in the brightness and color of the light, which helps define its various properties. The spectrum can reveal how much light is coming from the quasar. If there’s a significant difference, it’s a clear sign of change!

Surprises Await

One of the most fascinating aspects of these discoveries is how the changing behavior of these quasars can challenge our current understanding. For instance, while it was expected that Ly light would disappear first during the changing-look event, researchers found that another light type called C iv could still be present even after Ly light changed. It’s like one singer holding a note while another takes a vacation-unexpected and puzzling!

The Importance of Timing

The timing of these changing events is also crucial. It helps scientists understand how fast these processes are happening. The observed changes between J1306 and J1512 happened over a span of 1 to 3.5 years. Imagine waiting more than a year to see a new season of your favorite show, only to find that the characters have suddenly transformed!

A New Perspective on the Universe

These findings are not just about understanding individual quasars; they provide insight into how black holes function and evolve. They can also shed light on how galaxies interact and develop over time. It’s like piecing together a grand cosmic narrative, one quasar at a time.

Future Observations

More observations of these changing-look quasars will help scientists refine their ideas and theories. Researchers are particularly interested in using different wavelengths of light-like X-ray and infrared-to gain more clues about what’s happening inside these cosmic giants. Think of them as detectives gathering evidence from different crime scenes!

What Makes These Findings Unique

These quasars are not just any quasars; they are changing-look quasars that exist at high redshifts, which means they are very far away in the universe. Studying them can help unlock mysteries about the universe’s infancy and how galaxies have evolved over time.

Implications for Astronomy

Understanding changing-look quasars is essential for astronomers. It can help refine models about how black holes grow, how they consume material, and how they influence their surroundings. Knowledge gained from these findings can help inform many areas of astrophysics and cosmology.

The Bigger Picture

In the grand scheme of things, studying quasars and their changes can reshape our understanding of the universe. By learning how these powerful entities behave, we can gain a deeper appreciation of the complexity of galaxies, black holes, and cosmic evolution.

Conclusion

Changing-look quasars, particularly those recently discovered, provide a thrilling glimpse into the dynamic nature of the universe. They remind us that the cosmos is full of surprises, waiting to be explored. As researchers continue to observe these fascinating objects, we can expect more adventures in the world of astronomy. Just like in a good story, there are always new twists and turns waiting to be uncovered!

Original Source

Title: The first identification of Lyman $\alpha$ Changing-look Quasars at high-redshift in DESI

Abstract: We present two cases of Ly$\alpha$ changing-look (CL) quasars (J1306 and J1512) along with two additional candidates (J1511 and J1602), all discovered serendipitously at $z >2$ through the Dark Energy Spectroscopic Instrument (DESI) and the Sloan Digital Sky Survey (SDSS). It is the first time to capture CL events in Ly$\alpha$ at high redshift, which is crucial for understanding underlying mechanisms driving the CL phenomenon and the evolution of high-redshift quasars and galaxies. The variability of all four sources is confirmed by the significant change of amplitude in the $r$ band ($|r_{\rm DESI}-r_{\rm SDSS}| >0.5 \ \rm mag$). We find that the accretion rate in the dim state for these CL objects corresponds to a relatively low value ($\mathscr{\dot M} \approx 2\times10^{-3}$), which suggests that the inner region of the accretion disk might be in transition between the Advection Dominated Accretion Flow ($\mathscr{\dot M}

Authors: Wei-Jian Guo, Zhiwei Pan, Małgorzata Siudek, Jessica Nicole Aguilar, Steven Ahlen, Davide Bianchi, David Brooks, Todd Claybaugh, Kyle Dawson, Axel de la Macorra, Peter Doel, Kevin Fanning, Jaime E. Forero-Romero, Enrique Gaztañaga, Satya Gontcho A Gontcho, Klaus Honscheid, Robert Kehoe, Theodore Kisner, Andrew Lambert, Martin Landriau, Laurent Le Guillou, Marc Manera, Aaron Meisner, John Moustakas, Andrea Muñoz-Gutiérrez, Adam Myers, Jundan Nie, Nathalie Palanque-Delabrouille, Claire Poppett, Francisco Prada, Mehdi Rezaie, Graziano Rossi, Eusebio Sanchez, Michael Schubnelll, Hee-Jong Seo, Joseph Harry Silber, David Sprayberry, Gregory Tarlé, Benjamin Alan Weaver, Zhimin Zhou, Hu Zou

Last Update: 2024-11-04 00:00:00

Language: English

Source URL: https://arxiv.org/abs/2411.01949

Source PDF: https://arxiv.org/pdf/2411.01949

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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