The Unusual Twists of Galaxy 4C 70.19
4C 70.19 showcases unique twisted jets and intriguing cosmic interactions.
M. Weżgowiec, M. Jamrozy, K. T. Chyży, M. J. Hardcastle, A. Kuźmicz, G. Heald, T. W. Shimwell
― 7 min read
Table of Contents
- What’s a Radio Galaxy?
- Meet 4C 70.19
- The Research Process
- The Role of Magnetic Fields
- Discovery of Diffuse Emissions
- Estimating the Environment
- The Twists and Turns of the Jets
- The Size of 4C 70.19
- The Role of the Host Galaxy
- The Companions in the Neighborhood
- The Spectacle of the Radio Spectrum
- Conclusion: A Cosmic Mystery
- Original Source
- Reference Links
In the vast universe, there are many strange and wonderful phenomena. One such spectacle is a peculiar radio galaxy known as 4C 70.19. Located near a giant elliptical galaxy called NGC 6048, this radio galaxy has behaviors that leave scientists scratching their heads, much like trying to understand why your cat suddenly decides to chase its tail.
4C 70.19 is like that one friend who is always doing something unexpected. Instead of the usual straight Jets that many galaxies have, this one has twisted and bent jets, resembling more of a cosmic spaghetti than anything else. These jets shoot out from the central region of the galaxy, but they're not just randomly flailing about. There’s some evidence suggesting that they are interacting with their surroundings, leading to their unique shapes.
What’s a Radio Galaxy?
Before diving deeper into 4C 70.19, let’s clarify what a radio galaxy is. Essentially, these are galaxies that emit strong radio waves. Imagine a galaxy as a glowing blob in the universe, sending out signals like a cosmic radio station. The source of these signals is usually an active galactic nucleus (AGN), which is an area at the center of the galaxy that is incredibly bright and energetic.
The AGN can produce jets of particles that zoom out into space at nearly the speed of light. It’s like a cosmic fountain, but instead of water, you have highly energetic particles shooting out into the universe.
Meet 4C 70.19
Now, let’s return to our friend, 4C 70.19. It’s quite the oddball among Radio Galaxies. While many have symmetrical jets shooting out in pairs, this galaxy presents a different picture. Its jets are not only bent, but one of them even performs a dramatic 180-degree twist! It’s as if the jets have a flair for the theatrical.
This peculiar behavior isn’t just for show. The jets’ twisted paths suggest that they are influenced by their environment. Perhaps they are bending around a cosmic obstacle course made of gas and other galaxies.
So, what do these jets look like? Picture a pair of glowing, energetic streams that split from the galaxy. As they stretch out into space, one jet takes a sharp turn, creating a hook-like shape, while the other keeps a more traditional route but still deviates a bit. It’s like they are trying to navigate through a crowded space, avoiding invisible obstacles left and right.
The Research Process
To better understand 4C 70.19 and its twisted jets, researchers used various radio telescopes, including LOFAR, VLA, and Effelsberg, to collect data. LOFAR is like that friend who brings the best snacks to the party. It’s particularly good at picking up low-frequency signals, which is perfect for spotting faint emissions that other telescopes might miss.
Effelsberg and VLA provide higher frequency data, allowing scientists to dive deeper into the details of how the jets behave. Researchers also combined radio data with optical and X-ray observations to get a complete picture of the surroundings of 4C 70.19. It’s like putting on special glasses to see all the colors of a rainbow instead of just the basic shades.
Magnetic Fields
The Role ofOne of the exciting aspects of 4C 70.19 is its magnetic fields. Think of magnetic fields as invisible hands gently guiding the jets. Polarization data, which helps scientists understand how these magnetic fields are aligned, suggests that they are being sheared at the locations where the jets bend. This shearing is like giving the jets a cosmic haircut at the points where they twist.
The magnetic fields are crucial because they impact how the jets behave. They can compress or stretch the jets, causing the unique shapes we observe. Understanding these magnetic fields helps researchers figure out what’s happening in the galaxy’s environment and how it interacts with its surroundings.
Diffuse Emissions
Discovery ofDuring the study of 4C 70.19, researchers stumbled upon something unexpected: diffuse emissions surrounding the jets. These emissions act like a faint glow around the bright jets, reminiscent of fog wrapping around a city at night.
Using sensitive radio maps, scientists could see these previously unnoticed emissions. They provide insight into what’s happening beyond the main jets and can hint at how the jets interact with the intergalactic medium (the gas and dust between galaxies).
Estimating the Environment
To grasp the nature of the environment around 4C 70.19, researchers used rotation measures derived from the data. This is like taking a measurement of the air pressure around you to understand the weather. The density of the surrounding medium is estimated to be similar to values found in the intergalactic medium or the outer parts of stellar halos.
This estimated density helps scientists understand how the jets are influenced by the surrounding "cosmic ocean." If it’s too thick or turbulent, it could cause the jets to bend and twist in dramatic ways, much like how a boat struggles to move through choppy waters.
The Twists and Turns of the Jets
When analyzing 4C 70.19’s jets, researchers noted that the southern jet also bends, just like the northern one. However, this one leans more toward the sky plane, much like a toddler trying to see over a tall fence by stretching upward.
Both bends likely emerged from the orbital motion within the galaxy group and interactions with the intergalactic medium. It’s a cosmic performance where the jets are the dancers, and the environment plays the music guiding their movements.
The Size of 4C 70.19
Despite its complicated appearance, 4C 70.19 is believed to be intrinsically symmetric. It’s estimated to have a physical extent of up to 600 kiloparsecs (kpc). To give you an idea, one kiloparsec is about 3,262 light-years – so this thing is massive!
To put this into perspective, if 4C 70.19 were a city, it would stretch over vast distances, occupying space about 1.8 million light-years wide. Imagine trying to walk across the entire city without a map; it would take you quite some time!
The Role of the Host Galaxy
At the center of the show is the giant elliptical galaxy NGC 6048. This galaxy plays a crucial role in the behavior of 4C 70.19. While the jets are propelled outwards from the AGN in 4C 70.19, they are also influenced by the gravitational and energetic environment of the host galaxy.
NGC 6048 is like the parent in this story, providing guidance and sometimes causing a bit of chaos. The interaction between the jets and the host galaxy is a complex dance, with both parties affecting each other’s movements.
The Companions in the Neighborhood
4C 70.19 is not alone in the cosmic playground; it has neighbors-other galaxies that are part of its larger group. Some of these companions are relatively close; they could be described as cosmic next-door neighbors who might have a say in the goings-on of 4C 70.19.
Interactions between these galaxies can impact the jets' trajectories, making their paths even more convoluted. Think of it like a game of dodgeball-when one player throws the ball, it might hit others or cause unexpected ripples in the game’s dynamics.
The Spectacle of the Radio Spectrum
One of the phenomenal aspects of studying 4C 70.19 is analyzing its radio spectrum. This spectrum reveals how the brightness changes at different frequencies, providing insights into the activity occurring in the jets and lobes.
A flatter global spectral index indicates that both acceleration and re-acceleration processes play a significant role throughout the source. It’s as if the jets are like energy drinks, constantly recharging to keep going despite the vast distances they cover.
Conclusion: A Cosmic Mystery
As researchers continue to unveil the secrets of 4C 70.19, its twisted jets, diffuse emissions, and interaction with nearby galaxies remain a captivating cosmic mystery. Each observation adds another piece to the puzzle, creating a clearer picture of this intriguing galaxy.
The findings showcase the beauty and complexity of the universe. From bending jets to unseen emissions, 4C 70.19 is just another reminder that there is still so much to discover beyond our own little planet. The cosmos is alive, filled with unusual characters like 4C 70.19, ready to surprise us at every turn.
In the end, as we gaze into the night sky, we may just find ourselves pondering: what other eccentric galaxies are out there, waiting for their stories to be told? The universe is a vast stage, and each galaxy is a performer in this grand cosmic play.
Title: The twisted jets and magnetic fields of the extended radio galaxy 4C 70.19
Abstract: The appearance of the jets and lobes of some radio galaxies makes it difficult to assign them to a known class of objects. This is often due to the activity of the central engine and/or interactions with the environment, as well as projection effects. We analyse the radio data for an apparently asymmetric radio source 4C70.19, which is associated with the giant elliptical galaxy NGC6048. The source shows distorted radio jets and lobes, one of which bends by 180 degrees. The aim of our study is to explain the nature of the observed distortions. We used LOFAR, Effelsberg, and VLA radio data in a wide range of frequencies. At high frequencies, we also used radio polarimetry to study the properties of the magnetic fields. Additionally, we made use of optical, infra-red, and X-ray data. Polarisation data suggest shearing of the magnetic fields at points where the jets bend. The low-frequency LOFAR map at 145 MHz, as well as the sensitive single-dish Effelsberg map at 8.35 GHz, reveal previously undetected diffuse emission around the source. The rotation measure (RM) derived from the polarimetric data allowed us to estimate the density of the medium surrounding the source, which agrees with typical densities of the intergalactic medium or the outer parts of insterstellar halos. We propose that the southern jet is bent in the same manner as the northern one, but that it is inclined to the sky plane. Both these bends are likely caused by the orbital motion within the galaxy group, as well as interactions with the intergalactic medium. Our analyses suggest that, despite its complex morphology, 4C70.19 seems to be intrinsically symmetric with a physical extent of up to 600 kpc, and that the diffuse emission detected in our high-sensitivity maps is related to radio plumes that are expanding behind the source.
Authors: M. Weżgowiec, M. Jamrozy, K. T. Chyży, M. J. Hardcastle, A. Kuźmicz, G. Heald, T. W. Shimwell
Last Update: 2024-11-04 00:00:00
Language: English
Source URL: https://arxiv.org/abs/2411.02121
Source PDF: https://arxiv.org/pdf/2411.02121
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.