For more information:

William Steigerwald
NASA Goddard Space Flight Center
(Phone: 301/286-5017)

Chandra Observatory homepage

Caption for Image One: This Hubble "Wide Field Planetary Camera 2" image reveals the central region of M15, a globular cluster containing over 30,000 stars. Here we see the core, with about a thousand stars confined within the innermost 1.6 light years of the cluster. Images in ultraviolet, blue, and visual light were combined for this picture so that the colors roughly correspond to the surface temperatures of stars in M15. Hot stars appear blue, while cooler stars appear reddish-orange.

The Chandra observation involves two X-ray binary systems: One contains neutron star 4U2127 orbiting around normal star AC211, the latter of which can be seen as a blue star in this Hubble image. The other binary contains the newly named M15-X2 neutron star, likely associated with a second, unnamed blue star. Thus, this Hubble image had the necessary resolution to clearly differentiate between the two optical stars in question yet could not identify a neutron star binary systems, which are visible in X-ray radiation.

Credit: NASA/HST -- P. Guhathakurta (UCO/Lick Observatory, UC Santa Cruz), B. Yanny (Fermi National Accelerator Lab), D. Schneider (Pennsylvania State Univ.), J. Bahcall (Inst. for Advanced Study)

Caption for Image Two: What was once thought to be one X-ray source is really two sources separated by 2.7 arcseconds. (The distance across Mars, from our vantage point on Earth, forms an angle of about 5 arcseconds. So imagine a gap smaller than that pinpoint of light from Mars.)

The new X-ray source called M15-X2, likely a neutron star orbiting a faint blue star. Earlier observations found this "single" star system, then only known as neutron star 4U2127, to behave in entirely two different ways. The reason, finally revealed, is that there are indeed two different systems. Chandra, capable of 0.5 arcsecond imaging resolution, was the first X-ray satellite that could make sense of the source. The broader implication of the Chandra discovery is that these types of binaries (a neutron star orbiting another star) can be quite common in star clusters, as was theorized but never observed.

Credit: NASA/CXO/White, Angelini

Image 1 TIFF

Image 2 TIFF

Image 3 TIFF

Image 4 TIFF

The Top Story Archive listing can be found by clicking on this link.

All stories found on a Top Story page or the front page of this site have been archived from most to least current on this page.

For a list of recent press releases, click here.

September 06, 2001 - (date of web publication)

Mysterious "Twofaced" Star Explained, Scientists Say

	Image 1

There's a simple reason why a curious neutron star in the M15 globular star cluster has shown two faces over the years, beaming an X-ray portrait as perplexing as Mona Lisa's smile. The reason: That's not one star system, but two.

Scientists at NASA Goddard Space Flight Center in Greenbelt, Md., capitalized on the exquisite resolution afforded by the Chandra X-ray Observatory to find a second neutron-star binary source just a hair west of the first binary source. The sources had blended together in all earlier observations.

The broader implication of the Chandra discovery is that these types of binaries (a neutron star orbiting another star) can be quite common in star clusters, as was theorized but never observed. Drs. Nicholas White and Lorella Angelini of Goddard's Laboratory for High Energy Astrophysics present their findings today in Washington, D.C., at a conference entitled "Two Years of Science with Chandra".

"We had long assumed there should be more of these neutron star binary systems, and now we are finally finding them," says White. "Past observations of M15, seemingly contradictory, also now make sense in retrospect. The first neutron star is coy, completely hiding behind the swirl of gas that is falling on to it. The second neutron star is prone to outbursts in X-ray light that reveal the star's surface."

	Image 2

Previously, and inexplicably, astronomers had never seen more than one of these neutron star binaries, called low-mass X-ray inaries, in any given globular cluster, a tight spherical region crowded with stars. M15, a beautiful display containing over a million stars, is one of the largest globular clusters, located in the constellation Pegasus some 34,000 light years from Earth.

Astronomers discovered one neutron star system in M15, called 4U2127, with the Einstein X-ray satellite in 1984. Characteristic of a low-mass X-ray binary, 4U2127 contains a city-sized neutron star orbiting a "living" hydrogen-burning star slightly smaller than our Sun, named AC211. Escaped gas from AC211 falls onto the neutron star, attracted by its strong center of gravity. The transfer of gas, called an accretion disk, glows hot in X rays.

The data revealed that the neutron star itself was not directly visible in X-ray light because it was hidden behind the accretion disk. This neat picture was put into doubt when the Japanese Ginga X-ray satellite saw luminous X-ray bursts from the region in 1990. The length of the burst and other light characteristics implied that the surface of the neutron star was directly visible, a complete contradiction to earlier observations.

Using Chandra's HETGS instrument, White and Angelini observed the region for nearly six hours on August 24, 2000. Chandra is capable of 0.5 arcsecond imaging resolution, several times sharper than Einstein.

	Image 3

White and Angelini discovered that what was thought to be one X-ray source is really two sources separated by 2.7 arcseconds. The distance across Mars, from our vantage point on Earth, forms an angle of about 5 arcseconds. So imagine a gap smaller than that pinpoint of light from Mars.) The new X-ray source, which they dubbed M15-X2, is likely a neutron star orbiting a faint blue star, Angelini said.

Globular clusters, with their myriad stars, should contain several low-mass X-ray binary systems. The fact that there was never more than one seen in any globular cluster, including the massive M15, led some theorists to speculate that these binaries are short-lived. Or, perhaps neutron stars -- created from burned-out, collapsed stars during supernova explosions -- are ejected from globular clusters with a thunderous kick as the neutron stars forms.

	Image 4

The Chandra observation has eliminated the need for such elaborate scenarios. M15 has at least two low-mass X-ray binary systems, and perhaps multiple systems in other cluster will be discovered given advancements in X-ray resolution. Indeed, M15 also has many radio pulsars, which may be the remnants of low-mass X-ray binary systems.

Angelini joins NASA Goddard through the University Space Research Association. The Chandra HETGS, or High Energy Transmission Grating Spectrometer, was built by the Massachusetts Institute of Technology.

Back to Top