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Source: Space Telescope Science Institute (STScI) 

Space Telescope Science Institute (STScI)
  Released: Mon 11-Dec-2006, 18:30 ET 
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Heavyweight Stars Light Up Nebula NGC 6357

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HUBBLE SPACE TELESCOPE ADVANCED CAMERA FOR SURVEYS, PISMIS 24, NGC 6357

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NASA Hubble Space Telescope high-resolution images of a star previously believed to be amongst the heaviest known in our Milky Way show that it is really two stars orbiting one another. Originally, the mass of the star was thought to be an incredible 200-300 solar masses, but the mass is now found to be only 100 solar masses.

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Credit: NASA, ESA, and J. Maíz Apellániz (Instituto de Astrofísica de Andalucía, Spain)
NASA Hubble Space Telescope Advanced Camera for Surveys high-resolution images of the star Pismis 24-1 show that it is really two stars orbiting one another (inset pictures at top right and bottom right). The stars are estimated to each be 100 solar masses.
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Newswise — The small open star cluster Pismis 24 lies in the core of the large emission nebula NGC 6357 in Sagittarius, about 8,000 light-years away from Earth. Some of the stars in this cluster are extremely massive and emit intense ultraviolet radiation.

The brightest object in the picture is designated Pismis 24-1. It was once thought to weigh as much as 200 to 300 solar masses. This would not only have made it by far the most massive known star in the galaxy, but would have put it considerably above the currently believed upper mass limit of about 150 solar masses for individual stars.

However, Hubble Space Telescope high-resolution images of the star show that it is really two stars orbiting one another (inset pictures at top right and bottom right). They are estimated to each be 100 solar masses.

In addition, spectroscopic observations with ground-based telescopes further reveal that one of the stars is actually a tight binary that is too compact to be resolved even by Hubble. This divides the estimated mass for Pismis 24-1 among the three stars. Although the stars are still among the heaviest known, the mass limit has not been broken thanks to the multiplicity of the system.

The observations were performed by a team of astronomers led by Jesús Maíz Apellániz of the Instituto de Astrofísica de Andalucía in Spain. The team imaged Pismis 24-1 with Hubble's Advanced Camera for Surveys in April 2006.

The images of NGC 6357 were taken with Hubble's Wide Field and Planetary Camera 2 in April 2002.

Credit: NASA, ESA, and J. Maíz Apellániz (Instituto de Astrofísica de Andalucía, Spain)

Images and additional information about Pismis 24 are available on the Web at:
http://hubblesite.org/news/2006/54
http://www.spacetelescope.org/news/html/heic0619.html

The Hubble Space Telescope is a project of international cooperation between NASA and the European Space Agency (ESA). The Space Telescope Science Institute in Baltimore conducts Hubble science operations. The Institute is operated for NASA by the Association of Universities for Research in Astronomy, Inc., Washington.