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Clean clusters within NGC 1512 appear as bright blue clumps of ultraviolet and visible light. Clusters clouded by interstellar dust are revealed by the glow of the clouds in which they are hidden, as detected in infrared wavelengths (red).
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By Robert Roy Britt
Senior Science Writer
posted: 09:00 am ET
31 May 2001

An extensive, multi-wavelength study with the Hubble Space Telescope has shown the many faces of the galaxy NGC 1512

Infant stars in a nearby galaxy show themselves to be far more capable than human children of cleaning up after themselves.

A new Hubble Space Telescope image combines seven photographs in various wavelengths of light to reveal intense clusters of starbirth in a ring around galaxy NGC 1512. The clusters, it turns out, are either still mired in the clouds out of which they formed, or they have quickly cleaned things up and therefore shine brightly in visible light.

"The clusters are either completely hidden, enshrouded in their birth clouds, or almost completely exposed," said Dan Maoz of Tel Aviv University in Israel and Columbia University.

Astronomers already knew that stars are born out of giant clouds of gas and dust. Over time, the stars' own emissions help clear out leftover material. But in NGC 1512, the stellar nurseries are huge, and the cleansing process occurred with surprising rapidity.

"Apparently the winds from the young stars and the supernovae clear out the gas and the dust very quickly," Maoz told SPACE.com. "It happens over less than few million years."

In the new image, released today, clean clusters appear as bright blue clumps of ultraviolet and visible light. Clusters clouded by interstellar dust are revealed by the glow of the clouds in which they are hidden, as detected in infrared wavelengths and showing up on the image as red light permeating the dark, dusty lanes in the ring.

Beyond our galaxy

Maoz, who led a team that produced the images, said this cleansing process is understood, but not in detail. This is partly due to the fact that the most highly populated and energetic star clusters are outside our own galaxy.

"It is much better to study super star clusters in starburst galaxies, or galaxies like NGC 1512 with a starburst ring, where there can be hundreds of clusters," Maoz said. NGC 1512 is 30 million light-years away.

The research might help astronomers interpret similar observations of more distant galaxies, which are faint and therefore do not allow for such detailed images. Understanding starbirth in distant galaxies would provide a window to star formation when the universe was young.

"It is remarkable how similar the properties of this starburst are to those of other nearby starbursts that have been studied in detail with Hubble," said Aaron Barth, a Harvard-Smithsonian Center for Astrophysics researcher who also worked on creating the image.

The results will be published in the June issue of the Astronomical Journal.

Details of the galaxy and the image

NGC 1512 is known as a barred spiral galaxy, because of its rotating arms and a central bar loaded with matter (the bar is not visible in the new images). The giant bar in NGC 1512 is thought to funnel gas into the starburst ring.

The galaxy sits in the southern constellation of Horologium. It spans 70,000 light-years, nearly as much as our own Milky Way Galaxy, and is bright enough to be seen with amateur telescopes.

The new composite image was created from images taken with three different Hubble cameras, the Faint Object Camera (FOC), the Wide Field and Planetary Camera 2 (WFPC2) and the Near Infrared Camera and Multi-Object Spectrometer (NICMOS). The images were created in 1993, 1998 and 1999.

Hubble is operated by the Space Telescope Science Institute for NASA and the European Space Agency.

Click here for more Hubble news and pictures.

 

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