GPS News  
STELLAR CHEMISTRY
'Hyper-starburst' galaxy churns out stars, clues to universe's evolution
by Staff Writers
Gainesville FL (SPX) Dec 09, 2016


The distorted galaxy in the simulation results from a collision between two galaxies, followed by them merging. Astronomers think such a merger could be the reason why SPT0346-52 is having such a boom of stellar construction. Once the two galaxies collide, gas near the center of the merged galaxy (shown as the bright region in the center of the simulation) is compressed, producing a burst of new stars. The composite inset shows X-ray data from Chandra (blue), short wavelength infrared data from Hubble (green), infrared light from Spitzer (red) at longer wavelengths, and infrared data from ALMA (magenta) at even longer wavelengths. (The light from SPT0346-52 is distorted and magnified by the gravity of an intervening galaxy, producing three elongated images in the ALMA data located near the center of the image. SPT0346-52 is not visible in the Hubble or Spitzer data, but the intervening galaxy causing the gravitational lensing is detected.) There is no blue at the center of the image, showing that Chandra did not detect any X-rays that could have signaled the presence of a growing black hole. Image courtesy of CXC Press Office.

A recently discovered galaxy is undergoing an extraordinary boom of stellar construction, revealed by a group of astronomers led by University of Florida graduate student Jingzhe Ma using NASA's Chandra X-Ray Observatory. The galaxy known as SPT 0346-52 is 12.7 billion light years from Earth, seen at a critical stage in the evolution of galaxies about a billion years after the Big Bang.

Astronomers first discovered SPT 0346-52 with the National Science Foundation's South Pole Telescope, then observed it with space and ground-based telescopes. Data from the NSF/ESO Atacama Large Millimeter/submillimeter Array in Chile revealed extremely bright infrared emission, suggesting that the galaxy is undergoing a tremendous burst of star birth.

However, an alternative explanation remained: Was much of the infrared emission instead caused by a rapidly growing supermassive black hole at the galaxy's center? Gas falling towards the black hole would become much hotter and brighter, causing surrounding dust and gas to glow in infrared light. To explore this possibility, researchers used NASA's Chandra X?ray Observatory and CSIRO's Australia Telescope Compact Array, a radio telescope.

No X?rays or radio waves were detected, so astronomers were able to rule out a black hole being responsible for most of the bright infrared light.

"We now know that this galaxy doesn't have a gorging black hole, but instead is shining brightly with the light from newborn stars," Ma said. "This gives us information about how galaxies and the stars within them evolve during some of the earliest times in the universe."

Stars are forming at a rate of about 4,500 times the mass of the Sun every year in SPT0346-52, one of the highest rates seen in a galaxy. This is in contrast to a galaxy like the Milky Way that only forms about one solar mass of new stars per year.

"Astronomers call galaxies with lots of star formation 'starburst' galaxies," said UF astronomy professor Anthony Gonzalez, who co-authored the study. "That term doesn't seem to do this galaxy justice, so we are calling it a 'hyper-starburst' galaxy."

The high rate of star formation implies that a large reservoir of cool gas in the galaxy is being converted into stars with unusually high efficiency.

Astronomers hope that by studying more galaxies like SPT0346-52 they will learn more about the formation and growth of massive galaxies and the supermassive black holes at their centers.

"For decades, astronomers have known that supermassive black holes and the stars in their host galaxies grow together," said co-author Joaquin Vieira of the University of Illinois at Urbana?Champaign.

"Exactly why they do this is still a mystery. SPT0346-52 is interesting because we have observed an incredible burst of stars forming, and yet found no evidence for a growing supermassive black hole. We would really like to study this galaxy in greater detail and understand what triggered the star formation and how that affects the growth of the black hole."

SPT0346-52 is part of a population of strong gravitationally-lensed galaxies discovered with the SPT. It appears about six times brighter than it would without gravitational lensing, which enables astronomers to see more details than would otherwise be possible.


Comment on this article using your Disqus, Facebook, Google or Twitter login.


Thanks for being here;
We need your help. The SpaceDaily news network continues to grow but revenues have never been harder to maintain.

With the rise of Ad Blockers, and Facebook - our traditional revenue sources via quality network advertising continues to decline. And unlike so many other news sites, we don't have a paywall - with those annoying usernames and passwords.

Our news coverage takes time and effort to publish 365 days a year.

If you find our news sites informative and useful then please consider becoming a regular supporter or for now make a one off contribution.
SpaceDaily Contributor
$5 Billed Once


credit card or paypal
SpaceDaily Monthly Supporter
$5 Billed Monthly


paypal only


.


Related Links
University of Florida
Stellar Chemistry, The Universe And All Within It






Share this article via these popular social media networks
del.icio.usdel.icio.us DiggDigg RedditReddit GoogleGoogle

Previous Report
STELLAR CHEMISTRY
Amateur astronomer helps uncover secrets of unique pulsar binary system
Toronto, Canada (SPX) Dec 09, 2016
A professional astrophysicist and an amateur astronomer have teamed up to reveal surprising details about an unusual millisecond pulsar (MSP) binary system comprising one of the fastest-spinning pulsars in our Galaxy and its unique companion star. Their observations, to be published in the Astrophysical Journal in December, are the first to identify "star spots" on an MSP's companion star. ... read more


STELLAR CHEMISTRY
Soil pHertility mapped across the world

S. Korea expands cull to contain bird flu

Researchers use nuclear methods to study pest-resistance in corn

Surging methane emissions imperil climate goals

STELLAR CHEMISTRY
Further improvement of qubit lifetime for quantum computers

Stamping technique creates tiny circuits with electronic ink

3-D solutions to energy savings in silicon power transistors

Physicists decipher electronic properties of materials in work that may change transistors

STELLAR CHEMISTRY
Raytheon contracted to repair F/A-18 weapon assemblies

US State Dept approves slew of ME defense deals

China fighter jet claim 'untrue': Japan

U.S. Air Force taps Leidos for JMPS engineering services

STELLAR CHEMISTRY
Google self-driving car unit spins off as Waymo

Electric vehicle market footprint growing

China auto sales peak in November: group

US unveils 'V2V' plan for cars to talk to each other

STELLAR CHEMISTRY
China factory-gate inflation hits 5-year high

EU agrees tougher trade rules amid China row

China faces battle over market economy status

Trump tough talk on China worries US exporters

STELLAR CHEMISTRY
A roadmap for guiding development and conservation in the Amazon

Indonesia expands protection for peatlands, climate

Laser technique boosts aerial imaging of woodlands

Green groups pressure Spain over 'at risk' wetlands

STELLAR CHEMISTRY
Cloud formation: How feldspar acts as ice nucleus

What satellites can tell us about how animals will fare in a changing climate

Satellites, airport visibility readings shed light on troops' exposure to air pollution

ISRO launches earth observation satellite, Resourcesat-2A

STELLAR CHEMISTRY
New aspect of atom mimicry for nanotechnology applications

ANU demonstrates 'ghost imaging' with atoms

Supersonic spray yields new nanomaterial for bendable, wearable electronics

Researchers use acoustic waves to move fluids at the nanoscale









The content herein, unless otherwise known to be public domain, are Copyright 1995-2024 - Space Media Network. All websites are published in Australia and are solely subject to Australian law and governed by Fair Use principals for news reporting and research purposes. AFP, UPI and IANS news wire stories are copyright Agence France-Presse, United Press International and Indo-Asia News Service. ESA news reports are copyright European Space Agency. All NASA sourced material is public domain. Additional copyrights may apply in whole or part to other bona fide parties. All articles labeled "by Staff Writers" include reports supplied to Space Media Network by industry news wires, PR agencies, corporate press officers and the like. Such articles are individually curated and edited by Space Media Network staff on the basis of the report's information value to our industry and professional readership. Advertising does not imply endorsement, agreement or approval of any opinions, statements or information provided by Space Media Network on any Web page published or hosted by Space Media Network. General Data Protection Regulation (GDPR) Statement Our advertisers use various cookies and the like to deliver the best ad banner available at one time. All network advertising suppliers have GDPR policies (Legitimate Interest) that conform with EU regulations for data collection. By using our websites you consent to cookie based advertising. If you do not agree with this then you must stop using the websites from May 25, 2018. Privacy Statement. Additional information can be found here at About Us.