File:Fast Radio Burst Galaxies.jpg

Size of this preview: 600 × 600 pixels. Other resolutions: 240 × 240 pixels | 480 × 480 pixels.

Original file (800 × 800 pixels, file size: 122 KB, MIME type: image/jpeg)

Captions

English

Add a one-line explanation of what this file represents

Summary

DescriptionFast Radio Burst Galaxies.jpg	English: Hunting for the neighborhoods of enigmatic, fast radio bursts (FRBs), astronomers using the NASA/ESA Hubble Space Telescope tracked four of them to the spiral arms of the four distant galaxies shown in the image. The bursts are catalogued as FRB 190714, at top left; FRB 191001, at top right; FRB 180924, at bottom left; and FRB 190608, at bottom right. Because these radio pulses disappear in much less than the blink of an eye, researchers have had a hard time tracking down where they come from. The galaxies are far from Earth, appearing as they looked billions of years ago. With the help of Hubble's sharp vision, astronomers pinpointed the fast radio bursts' location (denoted by the dotted oval lines) to the galaxies' spiral arms. These galaxies are part of a survey to determine the origin of these brilliant flares, which can release as much energy in a thousandth of a second as the Sun does in a year. Identifying the radio bursts' location helped researchers narrow the list of possible FRB sources that can generate such prodigious tsunamis of energy. One of the leading possible explanations is a torrential blast from a young magnetar. Magnetars are a type of neutron star with extraordinarily powerful magnetic fields. The observations were made in ultraviolet and near-infrared light with Hubble's Wide Field Camera 3. The images were taken between November 2019 and April 2020.
Date	20 May 2021, 19:00:00
Source	https://esahubble.org/images/opo2110a/
Author	NASA, ESA, A. Mannings (UC Santa Cruz), W. Fong (Northwestern), A. Pagan (STScI)

Licensing

attribution

ESA/Hubble images, videos and web texts are released by the ESA under the Creative Commons Attribution 4.0 International license and may on a non-exclusive basis be reproduced without fee provided they are clearly and visibly credited. Detailed conditions are below; see the ESA copyright statement for full information. For images created by NASA or on the hubblesite.org website, or for ESA/Hubble images on the esahubble.org site before 2009, use the {{PD-Hubble}} tag.

Conditions:

The full image or footage credit must be presented in a clear and readable manner to all users, with the wording unaltered (for example: "ESA/Hubble"). Web texts should be credited to ESA/Hubble (except when used by media). The credit should not be hidden or disassociated from the image footage. Links should be active if the credit is online. See the usage rights Q&A section on the ESA copyright page for guidance.
ESA/Hubble materials may not be used to state or imply the endorsement by ESA/Hubble or any ESA/Hubble employee of a commercial product or service.
ESA/Hubble requests a copy of the product sent to them to be indexed in their archive.
If an image shows an identifiable person, using that image for commercial purposes may infringe that person's right of privacy, and separate permission should be obtained from the individual.
If images or visuals are changed significantly from the original work (apart from resizing, cropping), we suggest that the changes are mentioned after the credit line. For example "Original image by ESA/Hubble (M. Kornmesser), warping and recolouring by NN".

Notes:

Note that this general permission does not extend to the use of ESA/Hubble's logo, which shall remain protected and may not be used or reproduced without prior and individual written consent of ESA/Hubble.
Also note that music, scientific papers and code on the esahubble.org site are not released under this license and can not be used for non-ESA/Hubble products.
By reproducing ESA/Hubble material, in part or in full, the user acknowledges the terms on which such use is permitted.

This file is licensed under the Creative Commons Attribution 4.0 International license.

Attribution: ESA/Hubble

You are free:

to share – to copy, distribute and transmit the work
to remix – to adapt the work

Under the following conditions:

attribution – You must give appropriate credit, provide a link to the license, and indicate if changes were made. You may do so in any reasonable manner, but not in any way that suggests the licensor endorses you or your use.

File history

Click on a date/time to view the file as it appeared at that time.

	Date/Time	Thumbnail	Dimensions	User	Comment
current	15:34, 8 June 2021		800 × 800 (122 KB)	Pandreve (talk \| contribs)	Uploaded a work by NASA, ESA, A. Mannings (UC Santa Cruz), W. Fong (Northwestern), A. Pagan (STScI) from https://esahubble.org/images/opo2110a/ with UploadWizard

You cannot overwrite this file.

File usage on Commons

There are no pages that use this file.

File usage on other wikis

The following other wikis use this file:

Usage on en.wikipedia.org
- Fast radio burst

Metadata

This file contains additional information such as Exif metadata which may have been added by the digital camera, scanner, or software program used to create or digitize it. If the file has been modified from its original state, some details such as the timestamp may not fully reflect those of the original file. The timestamp is only as accurate as the clock in the camera, and it may be completely wrong.

Image title	Hunting for the neighborhoods of enigmatic, fast radio bursts (FRBs), astronomers using the NASA/ESA Hubble Space Telescope tracked four of them to the spiral arms of the four distant galaxies shown in the image. The bursts are catalogued as FRB 190714, at top left; FRB 191001, at top right; FRB 180924, at bottom left; and FRB 190608, at bottom right. Because these radio pulses disappear in much less than the blink of an eye, researchers have had a hard time tracking down where they come from. The galaxies are far from Earth, appearing as they looked billions of years ago. With the help of Hubble's sharp vision, astronomers pinpointed the fast radio bursts' location (denoted by the dotted oval lines) to the galaxies' spiral arms. These galaxies are part of a survey to determine the origin of these brilliant flares, which can release as much energy in a thousandth of a second as the Sun does in a year. Identifying the radio bursts' location helped researchers narrow the list of possible FRB sources that can generate such prodigious tsunamis of energy. One of the leading possible explanations is a torrential blast from a young magnetar. Magnetars are a type of neutron star with extraordinarily powerful magnetic fields. The observations were made in ultraviolet and near-infrared light with Hubble's Wide Field Camera 3. The images were taken between November 2019 and April 2020.
Author	Space Telescope Science Institute Office of Public Outreach
Credit/Provider	NASA, ESA, A. Mannings (UC Santa Cruz), W. Fong (Northwestern), A. Pagan (STScI)
Source	ESA/Hubble
Short title	Fast Radio Burst Galaxies
Usage terms	Creative Commons Attribution 4.0 International License
Date and time of data generation	19:00, 20 May 2021
JPEG file comment	Astronomers using NASA’s Hubble Space Telescope have traced the locations of five brief, powerful radio blasts to the spiral arms of five distant galaxies. Called fast radio bursts (FRBs), these extraordinary events generate as much energy in a thousandth of a second as the Sun does in 80 years. Because these transient radio pulses disappear in much less than the blink of an eye, researchers have had a hard time tracking down where they come from, much less determining what kind of object or objects is causing them. Therefore, most of the time, astronomers don’t know exactly where to look. Locating where these blasts are coming from, and in particular, what galaxies they originate from, is important in determining what kinds of astronomical events trigger such intense flashes of energy. The new Hubble survey of eight FRBs helps researchers narrow the list of possible FRB sources. Flash in the Night The first FRB was ever discovered in archived data recorded by the Parkes radio observatory on July 24, 2001. Since then astronomers have uncovered up to 1,000 FRBs, but they have only been able to associate roughly 15 of them to particular galaxies. “Our results are new and exciting. This is the first high-resolution view of a population of FRBs, and Hubble reveals that five of them are localized near or on a galaxy’s spiral arms,” said Alexandra Mannings of the University of California, Santa Cruz, the study’s lead author. “Most of the galaxies are massive, relatively young, and still forming stars. The imaging allows us to get a better idea of the overall host-galaxy properties, such as its mass and star-formation rate, as well as probe what’s happening right at the FRB position because Hubble has such great resolution.” In the Hubble study, astronomers not only pinned all of them to host galaxies, but they also characterized the types of locations within those galaxies. Hubble observed one of the FRB locations in 2017 and the other seven in 2019 and 2020. “We don’t know what causes FRBs, so it’s really important to use context when we have it," said team member Wen-fai Fong of Northwestern University in Evanston, Illinois. "This technique has worked very well for identifying the progenitors of other types of transients, such as supernovae and gamma-ray bursts. Hubble played a big role in those studies, too.” The galaxies in the Hubble study existed roughly 7 billion years ago and so astronomers are seeing the light from them as they were at about half of the current age of the universe. Many of them are as massive as our Milky Way. The observations were made in ultraviolet and near-infrared light with Hubble’s Wide Field Camera 3. Ultraviolet light traces the glow of young stars strung along a spiral galaxy’s winding arms. The researchers used the near-infrared images to calculate the galaxies’ mass and find where older populations of stars reside. Location, Location, Location The images display a diversity of spiral-arm structure, from tightly wound to more diffuse, revealing how the stars are distributed along these prominent features. A galaxy’s spiral arms trace the distribution of young, massive stars. However, the Hubble images reveal that the FRBs found near the spiral arms do not come from the very brightest regions, which blaze with the light from hefty stars. The images help support a picture that the FRBs likely do not originate from the youngest, most massive stars. These clues helped the researchers rule out some of the possible stellar objects thought to cause these brilliant flares, including the explosive deaths of the youngest, most massive stars, which generate gamma-ray bursts and some types of supernovae. Another unlikely source is the merger of neutron stars, the crushed cores of stars that end their lives in supernova explosions. These mergers take billions of years to occur and are usually found far from the spiral arms of older galaxies that are no longer forming stars. Magnetic Monsters The team’s Hubble results, however, are consistent with the leading model that FRBs originate from young magnetar outbursts. Magnetars are a type of neutron star with powerful magnetic fields. They’re called the strongest magnets in the universe, possessing a magnetic field that is 10 trillion times more powerful than a refrigerator door magnet. Astronomers last year linked observations of an FRB spotted in our Milky Way galaxy with a region where a known magnetar resides. “Owing to their strong magnetic fields, magnetars are quite unpredictable,” Fong explained. “In this case, the FRBs are thought to come from flares from a young magnetar. Massive stars go through stellar evolution and become neutron stars, some of which can be strongly magnetized, leading to flares and magnetic processes on their surfaces, which can emit radio light. Our study fits in with that picture and rules out either very young or very old progenitors for FRBs.” The observations also helped the researchers strengthen the association of FRBs with massive, star-forming galaxies. Previous ground-based observations of some possible FRB host galaxies did not as clearly detect underlying structure, such as spiral arms, in many of them. Astronomers, therefore, could not rule out the possibility that FRBs originate from a dwarf galaxy hiding underneath a massive one. In the new Hubble study, careful image processing and analysis of the images allowed researchers to rule out underlying dwarf galaxies, according to co-author Sunil Simha of the University of California, Santa Cruz. Although the Hubble results are exciting, the researchers say they need more observations to develop a more definitive picture of these enigmatic flashes and better pinpoint their source. “This is such a new and exciting field,” Fong said. “Finding these localized events is a major piece to the puzzle, and a very unique puzzle piece compared to what’s been done before. This is a unique contribution of Hubble.”
Software used	Adobe Photoshop 22.2 (Macintosh)
File change date and time	14:29, 10 May 2021
Date and time of digitizing	08:39, 20 January 2021
Date metadata was last modified	10:29, 10 May 2021
Unique ID of original document	xmp.did:1cd243ea-49eb-4040-a519-78c782f0a31f
Keywords	Fast Radio Burst Hosts
Contact information	outreach@stsci.edu https://esahubble.org ESA Office, Space Telescope Science Institute, 3700 San Martin Dr Baltimore, MD, 21218 United States 410-338-4444
IIM version	4

File:Fast Radio Burst Galaxies.jpg

Captions

Captions

Summary

Licensing

File history

File usage on Commons

File usage on other wikis

Metadata

Structured data

Items portrayed in this file

depicts

fast radio burst

copyright status

copyrighted

copyright license

Creative Commons Attribution 4.0 International

inception

20 May 2021

media type

image/jpeg

Navigation menu

File:Fast Radio Burst Galaxies.jpg

Captions

Captions

Summary

Licensing

File history

File usage on Commons

File usage on other wikis

Metadata

Navigation menu

Search