Cygnus X-1: Still a 'Star' After All Those Years

August 28, 2009
Credits: NASA/CXC

Since its discovery 45 years ago, Cygnus X-1 has been one of the most intensively studied cosmic X-ray sources. About a decade after its discovery, Cygnus X-1 secured a place in the history of astronomy when a combination of X-ray and optical observations led to the conclusion that it was a black hole, the first such identification.

The Cygnus X-1 system consists of a black hole with a mass about 10 times that of the Sun in a close orbit with a blue supergiant star with a mass of about 20 Suns. Gas flowing away from the supergiant in a fast stellar wind is focused by the black hole, and some of this gas forms a disk that spirals into the black hole. The gravitational energy release by this infalling gas powers the X-ray emission from Cygnus X-1.

Although more than a thousand scientific articles have been published on Cygnus X-1, its status as a bright and nearby black hole continues to attract the interest of scientists seeking to understand the nature of and how they affect their environment. Observations with Chandra and ESA's are especially valuable for studying the property of the stellar wind that fuels Cygnus X-1, and determining its rate of spin.

This latter research has revealed that Cygnus X-1 is spinning very slowly. This puzzling result could indicate that Cygnus X-1 may have formed in an unusual type of that somehow prevented the newly formed black hole from acquiring as much spin as other stellar black holes.

Provided by JPL/NASA (news : web)

Explore further: Black Hole Blows Bubble Between The Stars

Related Stories

Black Hole Blows Bubble Between The Stars

August 11, 2005

A team of astronomers from The Netherlands and the UK has discovered a vast "jet-powered bubble" formed in the gas around a black hole in the Milky Way.

Recommended for you

A blue, neptune-size exoplanet around a red dwarf star

November 25, 2015

A team of astronomers have used the LCOGT network to detect light scattered by tiny particles (called Rayleigh scattering), through the atmosphere of a Neptune-size transiting exoplanet. This suggests a blue sky on this world ...

The hottest white dwarf in the Galaxy

November 25, 2015

Astronomers at the Universities of Tübingen and Potsdam have identified the hottest white dwarf ever discovered in our Galaxy. With a temperature of 250,000 degrees Celsius, this dying star at the outskirts of the Milky ...

Aging star's weight loss secret revealed

November 25, 2015

A team of astronomers using ESO's Very Large Telescope has captured the most detailed images ever of the hypergiant star VY Canis Majoris. These observations show how the unexpectedly large size of the particles of dust surrounding ...


Adjust slider to filter visible comments by rank

Display comments: newest first

not rated yet Aug 28, 2009
There's lots of scenarios that may spin-up a black-hole progenitor. What will make them spin-down ? Interaction of mag field with surrounds ?
not rated yet Aug 29, 2009
Tidal deceleration.
not rated yet Aug 29, 2009
Is the visible component -the blue supergiant- the star known as HDE226868? Or am I confusing X-ray sources?
not rated yet Aug 30, 2009
@birger, yes, indeed the blue supergiant is a.k.a. HD 226868, V1367 Gyg, BD 35 3815, among many other catalog numbers :)

Please sign in to add a comment. Registration is free, and takes less than a minute. Read more

Click here to reset your password.
Sign in to get notified via email when new comments are made.