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Circinus X-1
Circinus X-1
(25 Apr 00)
Cygnus X-3:
Chandra Shows New Way to Measure Cosmic Distances

Cygnus X-3

A team of scientists have used Chandra to observe a halo around the X-ray source Cygnus X-3. The halo (beyond the yellow ring in the center) is due to scattering by interstellar dust grains along the line of sight to the source. The sharp horizontal line is an instrumental effect.

The X-ray emission from Cygnus X-3 is due to matter falling from a normal star onto a nearby neutron star or black hole. Its X-ray emission varies regularly with a 4.8 hour period, as the compact star circles a companion star.

The radiation from the halo is delayed and smeared out, so the variations are damped. By observing the delays and smearing at different parts of the halo, the distance to the X-ray source is found to be 30,000 light years.

Fast Facts for Cygnus X-3:
Scale  Image is 200 arcsec across.
Category  Neutron Stars/X-ray Binaries
Coordinates (J2000)  RA 20h 32m 25.50s | Dec +40° 57' 27.70"
Constellation  Cygnus
Observation Dates  December 19, 1999
Observation Time  4 hours
Obs. IDs  1456
Color Code  Intensity
Instrument  ACIS
References P. Predehl et al, Astron. & Astrophys. (2000, in press)
Distance Estimate  30,000 light years
Release Date  April 25, 2000