. 24/7 Space News .
STELLAR CHEMISTRY
ASU astronomer finds star fuel surrounding galaxies
by Karin Valentine for ASU News
Tempe AZ (SPX) Jan 20, 2022

Illustration of the faint fuel reservoirs that surround galaxies, allowing them to form new stars and planetary systems. Image by Shireen Dooling/ASU

Most galaxies, including our own, grow by accumulating new material and turning them into stars - that much is known. What has been unknown is where that new material comes from and how it flows into galaxies to create stars.

In a recently published study, Arizona State University astronomer Sanchayeeta Borthakur has identified the faint fuel reservoirs that surround galaxies, and how this fuel can fall into galaxies, allowing them to form new stars and planetary systems. Her research has been published in the American Astronomical Society's Astrophysical Journal.

Previous research in the field of star formation suggested that some galaxies are producing more stars than what their reserve of star-forming gas would allow. This implied to Borthakur, who is an assistant professor at ASU's School of Earth and Space Exploration, that new gas must be coming into the galaxies and supporting the formation of new stars and planets.

"Observations of galaxies are similar to looking through an airplane window at night and seeing bright city lights surrounded by darkness. Finding this fuel source is like discovering that in the darkness lies the farms and supply routes that support the populations in the cities," explains Borthakur.

To determine where the gas might be originating, Borthakur used a statistical method known as cross-correlation (to measure the association between two quantities), and data from two publicly available astronomy catalogues: the ALFALFA survey from the Arecibo telescope and the Survey of the Low-Redshift Intergalactic Medium from the Hubble Space Telescope's Cosmic Origins Spectrograph. With those data, she was able to quantify how gas-rich galaxies are associated with clouds seen in the intergalactic medium.

"It's like discovering the existence and the location of gas stations in an image of a city full of vehicles," says Borthakur.

For next steps, she hopes to identify the pathways through which these gas clouds can reach the inner regions of the galaxies where stars are formed.

"Galaxies like ours will continue to grow by forming many more solar systems as new material comes in," she says. "Understanding the source of the star fuel allows us to predict if new stars will be formed in the future."

Research Report: "How are Lya Absorbers in the Cosmic Web Related to Gas-rich Galaxies"


Related Links
School of Earth and Space Exploration at ASU
Stellar Chemistry, The Universe And All Within It


Thanks for being there;
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 Monthly Supporter
$5+ Billed Monthly


paypal only
SpaceDaily Contributor
$5 Billed Once


credit card or paypal


STELLAR CHEMISTRY
Researchers Observe Massive CME on Distant, Sun-Like Star
Washington DC (SPX) Jan 14, 2022
EK Draconis illuminates an unimagined picture of how superflares may affect interplanetary space through coronal mass ejections Welcome to the New Year! While Earth celebrated 2022's arrival with displays of fireworks, the greatest "fireworks show" in our solar system often occurs on the Sun. Its atmosphere is a venue for dynamic sunspots, solar flares, and dramatic encores of released magnetic tension casting plasma particles into the cosmos via coronal mass ejections (CME). We've seen and studi ... read more

Comment using your Disqus, Facebook, Google or Twitter login.



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

STELLAR CHEMISTRY
NASA Solar Sail Mission to Chase Tiny Asteroid After Artemis I Launch

NASA Offers $1 Million for Innovative Systems to Feed Tomorrow's Astronauts

Russian cosmonauts conduct EVA to complete Nauka Lab Module integration to ISS

Five Space Station Research Results Contributing to Deep Space Exploration

STELLAR CHEMISTRY
NASA prepares final rocket tests for first Artemis moon mission launch

SpaceX ISS freighter splashes down off Florida

Ariane 6 upper stage readies for tests at Europe's Spaceport

Arianespace to launch Microcarb on Vega C

STELLAR CHEMISTRY
Sols 3362-3363: Sedimentologist's Delight

New control technique uses solar panels to reach desired Mars orbit

Hope for present-day Martian groundwater dries up

Consistent asteroid showers rock previous thinking on Mars craters

STELLAR CHEMISTRY
China's rocket technology hits the ski slopes

China conducts its first rocket launch of 2022

Shouzhou XIII crew finishes cargo spacecraft, space station docking test

China to complete building of space station in 2022

STELLAR CHEMISTRY
OneWeb and Hughes to bring orbital broadband service to India

Summit to ignite Europe's bold space ambitions

Advances in Space Transportation Systems Transforming Space Coast

AGIS signs Kleos' data evaluation contract

STELLAR CHEMISTRY
China satellite in close encounter with Russian debris: state media

Future trillion dollar 'space economy' threatened by debris, WVU researcher says

Lion will roam above the planet - KP Labs to release their "king of orbit"

Facebook trumpets massive new supercomputer

STELLAR CHEMISTRY
A planetary dynamical crime scene at 14 Herculis

TESS Science Office at MIT hits milestone of 5,000 exoplanet candidates

SETI's plan for a sky-monitoring telescope on the moon

Newly-Found Planets On The Edge Of Destruction

STELLAR CHEMISTRY
Oxygen ions in Jupiter's innermost radiation belts

Ocean Physics Explain Cyclones on Jupiter

Looking Back, Looking Forward To New Horizons

Testing radar to peer into Jupiter's moons









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.