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Quasars: A Look into Cosmic Brightness

Exploring quasars and their impact on the universe.

Avinanda Chakraborty, Maitreya Kundu, Suchetana Chatterjee, Swayamtrupta Panda, Arijit Sar, Sandra Jaison, Ritaban Chatterjee

― 5 min read


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Table of Contents

Quasars are some of the brightest and farthest objects in the universe. They are powered by supermassive black holes that gobble up nearby material and spit out tons of energy in the process. Imagine these black holes as cosmic vacuum cleaners, attracting everything in their vicinity and turning it into a starry show. In this piece, we will explore the different types of quasars, how scientists study them, and what they tell us about the universe.

What Are Quasars?

Quasars, short for "quasi-stellar objects," are incredibly luminous. They are not just any distant star; they are more like the rock stars of the cosmos. A quasar can shine brighter than entire galaxies! Their brightness comes from the gravitational energy released as matter falls into the black hole at their center. While they can emit radiation across the entire spectrum, from radio waves to X-rays, they are often categorized into two groups: radio-loud and Radio-Quiet Quasars.

  1. Radio-Loud Quasars: These guys are like the loud neighbors who love to blast music. They have strong radio emissions and are often associated with powerful jets-streams of particles blasted out into space at nearly the speed of light.

  2. Radio-Quiet Quasars: On the flip side, radio-quiet quasars are the quieter neighbors. They emit much less radio energy, making them harder to detect in that spectrum.

The Quasar Dilemma

So, what’s the big deal about these two groups? For many years, scientists have been scratching their heads trying to figure out why some quasars are radio-loud while others are radio-quiet. It's like trying to understand why some people prefer tea while others are die-hard coffee fans. Various theories have popped up, suggesting that differences in black hole mass, accretion rates, and star formation could hold the answers. However, no one theory has emerged victorious, leaving scientists with plenty of questions.

What’s Going On With the Host Galaxies?

To get a clearer view of quasars, scientists also look at their host galaxies. Picture the quasar as a celebrity and its host galaxy as the town where they live. The properties of these galaxies can affect how quasars behave. As galaxies have their own life cycles, the conditions in a host galaxy can influence the quasar's activity.

Building a Sample

To investigate this further, researchers used a list of quasars from a large database. The researchers focused on quasars with broad emission lines in their spectra-these lines are like the fingerprints of the quasar, revealing important information about its composition and behavior. They looked closely at both radio-loud and radio-quiet quasars to see if there were any physical differences related to their host galaxies.

Image and Data Collection

Using a variety of tools, including space telescopes, researchers collected data across different wavelengths of light-from X-rays to radio waves. This data acts like a cosmic jigsaw puzzle that helps put together the full picture of what’s happening with quasars and their galaxies.

Modeling the Quasar Spectrum

To understand the data, scientists often create models that simulate what the quasar's spectral energy distribution (SED) would look like. Think of it as creating a digital avatar that represents all the light emitted by the quasar across various wavelengths. These models help researchers determine key characteristics of the quasar and its host galaxy.

Star Formation Rates and Other Factors

The SED modeling gives insight into several important factors, like the star formation rate (SFR) in the host galaxy and the mass of stars present. By examining these aspects, scientists can make conclusions about how the quasar's activity affects the surrounding galaxy.

The Results Are In!

Upon analyzing the data, researchers found that the luminosity emitted from the host galaxies was significant-about 20% to 35% of the total luminosity observed. This means that while quasars are powerhouses of energy, their host galaxies still contribute a decent amount of light.

Comparing Radio-Loud and Radio-Quiet

When comparing the characteristics of radio-loud and radio-quiet quasars, researchers found some similarities and differences. For example, both types had similar values for stellar mass and dust luminosity. However, radio-quiet quasars tended to have older star populations and longer e-folding times than their radio-loud neighbors.

A Closer Look at Main Sequence Relations

One interesting finding was that the main sequence relations-the expected correlation between stellar mass and star formation-were different for the two groups. Radio-loud quasars tended to stray from the expected path, suggesting that something unique might be happening in their host galaxies, possibly due to the effects of powerful jets.

The Radio Dichotomy Problem

The study delves into the ongoing radio dichotomy issue in quasars. Why do some quasars have strong radio emissions while others do not? The findings suggest that lower Eddington Ratios-essentially a measure of how efficiently the black hole is accreting material-might be linked to decreased star formation rates in their host galaxies.

The Bigger Picture

The results from this research provide an independent avenue for examining the radio dichotomy from a host galaxy perspective. This helps to clarify how the cosmic dance between quasars and their host galaxies unfolds.

Future Prospects

As the field of quasar research continues to grow, scientists are eager to gather even more data and insights. Future studies will likely focus on various aspects, such as how environmental factors affect star formation in quasar host galaxies. So, stay tuned, as the quasar saga is far from over!

Conclusion

Quasars are fascinating celestial objects that serve as cosmic beacons, illuminating our understanding of the universe. By studying both the quasars and their host galaxies, researchers are piecing together the story behind these luminous objects. Through careful modeling and data collection, we’re beginning to unravel the mysteries of why some quasars are noisy while others are, well, not. Like a good detective story in space, the more we learn, the more questions arise, but that’s what makes the journey of scientific discovery so exciting!

Original Source

Title: Spectral Energy Distribution Modeling of Broad Emission Line Quasars: From X-ray to Radio Wavelengths

Abstract: We study the differences in physical properties of quasar-host galaxies using an optically selected sample of radio loud (RL) and radio quiet (RQ) quasars (in the redshift range 0.15 < z < 1.9) which we have further cross-matched with the VLA-FIRST survey catalog. The sources in our sample have broad Hbeta and MgII emission lines (1000 km/s < FWHM < 15000 km/s) with a subsample of high broad line quasars (FWHM > 15000 km/s). We construct the broadband spectral energy distribution (SED) of our broad line quasars using multi-wavelength archival data and targeted observations with the AstroSat telescope. We use the state-of-the-art SED modeling code CIGALE v2022.0 to model the SEDs and determine the best-fit physical parameters of the quasar host galaxies namely their star-formation rate (SFR), main-sequence stellar mass, luminosity absorbed by dust, e-folding time and stellar population age. We find that the emission from the host galaxy of our sources is between 20%-35% of the total luminosity, as they are mostly dominated by the central quasars. Using the best-fit estimates, we reconstruct the optical spectra of our quasars which show remarkable agreement in reproducing the observed SDSS spectra of the same sources. We plot the main-sequence relation for our quasars and note that they are significantly away from the main sequence of star-forming galaxies. Further, the main sequence relation shows a bimodality for our RL quasars indicating populations segregated by Eddington ratios. We conclude that RL quasars in our sample with lower Eddington ratios tend to have substantially lower star-formation rates for similar stellar mass. Our analyses, thus, provide a completely independent route in studying the host galaxies of quasars and addressing the radio dichotomy problem from the host galaxy perspective.

Authors: Avinanda Chakraborty, Maitreya Kundu, Suchetana Chatterjee, Swayamtrupta Panda, Arijit Sar, Sandra Jaison, Ritaban Chatterjee

Last Update: 2024-11-24 00:00:00

Language: English

Source URL: https://arxiv.org/abs/2411.15836

Source PDF: https://arxiv.org/pdf/2411.15836

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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