Space Industry and Business News  
STELLAR CHEMISTRY
Spinning stars shed new light on strange galactic signal
by Staff Writers
Canberra, Australia (SPX) May 01, 2022

The Galactic Centre Excess is an unexpected concentration of gamma-rays emerging from the centre of our galaxy that has long puzzled astronomers

Researchers from The Australian National University (ANU) have found an alternative explanation for a mysterious gamma-ray signal coming from the centre of the galaxy, which was long claimed as a signature of dark matter.

Gamma-rays are the form of electromagnetic radiation with the shortest wavelength and highest energy.

Co-author of the study Associate Professor Roland Crocker said this particular gamma-ray signal - known as the Galactic Centre Excess - may actually come from a specific type of rapidly-rotating neutron star, the super-dense stellar remnants of some stars much more massive than our sun.

The Galactic Centre Excess is an unexpected concentration of gamma-rays emerging from the centre of our galaxy that has long puzzled astronomers.

"Our work does not throw any doubt on the existence of the signal, but offers another potential source," Associate Professor Crocker said.

"It is based on millisecond pulsars - neutron stars that spin really quickly - around 100 times a second.

"Scientists have previously detected gamma-ray emissions from individual millisecond pulsars in the neighbourhood of the solar system, so we know these objects emit gamma-rays. Our model demonstrates that the integrated emission from a whole population of such stars, around 100,000 in number, would produce a signal entirely compatible with the Galactic Centre Excess."

The discovery may mean scientists have to re-think where they look for clues about dark matter.

"The nature of dark matter is entirely unknown, so any potential clues garner a lot of excitement," Associate Professor Crocker said.

"But our results point to another important source of gamma-ray production.

"For instance, the gamma-ray signal from Andromeda, the next closest large galaxy to our own may be mostly due to millisecond pulsars."

ANU Masters student Anuj Gautam led the research, which also involved scientists from The Australian Defence Force Academy, University of Canterbury, and University of Tokyo.??

Research Report:Millisecond pulsars from accretion-induced collapse as the origin of the Galactic Centre gamma-ray excess signal


Related Links
Australian National University
Stellar Chemistry, The Universe And All Within It


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


STELLAR CHEMISTRY
Giant stars undergo dramatic weight loss program
Sydney, Australia (SPX) Apr 15, 2022
Astronomers at the University of Sydney have found a slimmer type of red giant star for the first time. These stars have undergone dramatic weight loss, possibly due to the presence a greedy neighbour. Published in Nature Astronomy, the discovery is an important step forward to understanding the life of stars in the Milky Way - our closest stellar neighbours. There are millions of 'red giant' stars found in our galaxy. These cool and luminous objects are what our Sun will become in four billion ye ... 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
Astroscale's ELSA-d completes complex rendezvous operation

Cosmic Shielding to test Plasteel radiation shielding aboard Space Forge satellite

How can we reduce the carbon footprint of global computing?

In Scandinavia, wooden buildings reach new heights

STELLAR CHEMISTRY
Northrop Grumman Australia team brings together space capabilities for JP9102

DARPA seeks ionospheric insights to improve communication across domains

NASA and industry to collaborate on space communications initiative

NASA awards SpaceX, 5 other companies $278.5M for new comms satellites

STELLAR CHEMISTRY
STELLAR CHEMISTRY
China Satellite Navigation Conference to highlight digital economy, intelligent navigation

406 Day: how Galileo helps save lives

NASA uses moonlight to improve satellite accuracy

Identifying RF and GPS interferences for military applications with satellite data

STELLAR CHEMISTRY
Denmark, Sweden summoning Russian envoys over airspace breaches

Turkey air force pulls out of exercise in Athens; Says Greek jets violating airpsace

magniX teams aims to accelerate electric flight for commercial aviation

Lignin-based jet fuel packs more power for less pollution

STELLAR CHEMISTRY
New approach may help clear hurdle to large-scale quantum computing

Neon ice shows promise as new qubit platform

The quest for an ideal quantum bit

Kenya's e-waste recyclers battle to contain rising scourge

STELLAR CHEMISTRY
Keeper of the winds shines on

BRICS forum on big data for sustainable development held in Beijing

BRICS to use big data to achieve sustainable development goals

NASA's EMIT will map tiny dust particles to study big climate impacts

STELLAR CHEMISTRY
Costa Rica president-elect says will not ratify environment treaty

Bacteria can stick to plastic in the deep sea to travel around the ocean

Choking and sweating around Delhi's burning hill of trash

South Asia wilts in heat as Delhi rubbish dump burns









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.