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- ROSAT Observes Hot Gas in a Small Galaxy Group STSCI-93-05
-
- A visible light picture of a three galaxies known as NGC 2300 group,
- combined with a false-color image (magenta), taken in X-ray light with
- the ROSAT (an acronym for Roentgen Satellite, a joint project of
- Germany, the U.S.A., and the U.K.) satellite.
-
- The x-ray image, taken on April 25-27, 1992 with ROSAT's Position
- Sensitive Proportional Counter instrument, shows that the small group
- of galaxies is immersed in a huge cloud of hot gas, about 1.3 million
- light-years in diameter. Astronomers estimate that the cloud has a mass
- equal to 500 billion times that of the Sun, and is at a temperature of
- about 10 million kelvins (about 18 million degrees Fahrenheit).
-
- Although such gaseous material has previously been seen in rich
- clusters of galaxies, this is the first time such a hot medium has been
- found in a small group that is typical of most clusters in the
- universe.
-
- The existence of this gaseous envelope allows astronomers to measure
- the total mass of the system. The surprising result is that the total
- amount of material in the group is much larger than the sum of the mass
- of the hot gas and the stars in the galaxies. This means that a
- substantial amount of invisible "dark matter" envelops the system,
- keeping the hot gas contained.
-
- The NGC 2300 group is located about 150 million light-years from Earth
- in the direction of the northern circumpolar constellation Cepheus.
-
- Credit: John Mulchaey (STScI)
- David S. Davis (NASA GSFC and Univ. of MD)
- Dr. Richard F. Mushotzky (NASA GSFC)
- Dr. David Burstein (ASU)
-