A starburst with the prospect of gravitational waves (Update)

August 11, 2017 by Lee Mohon
Credit: X-ray: NASA/CXC/UMass Lowell/S. Laycock et al.; Optical: Bill Snyder Astrophotography

In 1887, American astronomer Lewis Swift discovered a glowing cloud, or nebula, that turned out to be a small galaxy about 2.2 million light years from Earth. Today, it is known as the "starburst" galaxy IC 10, referring to the intense star formation activity occurring there.

More than a hundred years after Swift's discovery, astronomers are studying IC 10 with the most powerful telescopes of the 21st century. New observations with NASA's Chandra X-ray Observatory reveal many pairs of that may one day become sources of perhaps the most exciting cosmic phenomenon observed in recent years: gravitational waves.

By analyzing Chandra observations of IC 10 spanning a decade, astronomers found over a dozen and neutron stars feeding off gas from young, massive stellar companions. Such double star systems are known as "X-ray binaries" because they emit large amounts of X-ray light. As a massive star orbits around its compact companion, either a black hole or neutron star, material can be pulled away from the giant star to form a disk of material around the compact object. Frictional forces heat the infalling material to millions of degrees, producing a bright X-ray source.

When the massive companion star runs out fuel, it will undergo a catastrophic collapse that will produce a supernova explosion, and leave behind a black hole or neutron star. The end result is two compact objects: either a pair of black holes, a pair of , or a black hole and neutron star. If the separation between the compact objects becomes small enough as time passes, they will produce gravitational waves. Over time, the size of their orbit will shrink until they merge. LIGO has found three examples of black hole pairs merging in this way in the past two years.

Starburst galaxies like IC 10 are excellent places to search for X-ray binaries because they are churning out stars rapidly. Many of these newly born stars will be pairs of young and . The most massive of the pair will evolve more quickly and leave behind a black hole or a neutron star partnered with the remaining massive star. If the separation of the stars is small enough, an X-ray binary system will be produced.

This new composite image of IC 10 combines X-ray data from Chandra (blue) with an optical image (red, green, blue) taken by amateur astronomer Bill Snyder from the Heavens Mirror Observatory in Sierra Nevada, California. The X-ray sources detected by Chandra appear as a darker blue than the stars detected in optical light.

The young stars in IC 10 appear to be just the right age to give a maximum amount of interaction between the massive stars and their compact companions, producing the most X-ray sources. If the systems were younger, then the massive stars would not have had time to go supernova and produce a neutron star or black hole, or the orbit of the massive star and the compact object would not have had time to shrink enough for mass transfer to begin. If the star system were much older, then both compact objects would probably have already formed. In this case transfer of matter between the compact objects is unlikely, preventing the formation of an X-ray emitting disk.

Chandra detected 110 X-ray sources in IC 10. Of these, over forty are also seen in optical light and 16 of these contain "blue supergiants", which are the type of young, massive, hot stars described earlier. Most of the other sources are X-ray binaries containing less massive stars. Several of the objects show strong variability in their X-ray output, indicative of violent interactions between the compact stars and their companions.

A pair of papers describing these results were published in the February 10th, 2017 issue of The Astrophysical Journal and is available online here and here. The authors of the study are Silas Laycock from the UMass Lowell's Center for Space Science and Technology (UML); Rigel Capallo, a graduate student at UML; Dimitris Christodoulou from UML; Benjamin Williams from the University of Washington in Seattle; Breanna Binder from the California State Polytechnic University in Pomona; and, Andrea Prestwich from the Harvard-Smithsonian Center for Astrophysics in Cambridge, Mass.

Explore further: Arp 299: Galactic Goulash

More information: The X-ray Binary Population of the Nearby Dwarf Starburst Galaxy IC 10: Variable and Transient X-ray Sources. arXiv. arxiv.org/abs/1611.08611

Blue Supergiant X-ray Binaries in the Nearby Dwarf Galaxy IC 10. arXiv. arxiv.org/abs/1701.03803

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1 / 5 (6) Aug 11, 2017
These faerie tales they conjure up to explain the binaries is little more than imaginary conjecture. There are electric currents that arise between the two stars of binaries (one likely birthed/ejected from the parent star) and the evidence are the X-rays detected of the discharges occurring between the two stars.
5 / 5 (7) Aug 11, 2017
There are electric currents that arise between the two stars of binaries (one likely birthed/ejected from the parent star) and the evidence are the X-rays detected of the discharges occurring between the two stars.
Welcome to Wal-Mart science 101, folks...
Captain Stumpy
5 / 5 (2) Aug 11, 2017
another WTF moment from the pseudoscience eu cult!
There are electric currents that arise between the two stars of binaries
@nazi sympathizing idiot pseudoscience eu cult peon
please show the theory based on validated science that is falsifiable from the eu cult that makes predictions that can and have been observed showing the electric currents between stars, etc

to date, the only predicitons the eu cult has made have been falsified and proven garbage http://phys.org/n...oon.html



then also show the empirical evidence and measurements for the electric currents between stars, as well as your above binary star measurements

lastly: do not link your pseudoscience site
if you can't provide reputable science then you're delusional and it's the equivalent of pissing into a fan and calling it rain
not rated yet Aug 12, 2017
Stumpy you are so foul and reprehensible.

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