Image: The Heart of a Rose

Sep 08, 2010
Credit: X-ray (NASA/CXC/SAO/J. Wang et al), Optical (DSS & NOAO/AURA/NSF/KPNO 0.9-m/T. Rector et al)

(PhysOrg.com) -- This composite image shows the Rosette star formation region, located about 5,000 light years from Earth.

Data from the are colored red and outlined by a white line (roll your mouse over the image above). The X-rays reveal hundreds of in the central cluster and fainter clusters on either side. Optical data from the and the Kitt Peak National Observatory (purple, orange, green and blue) show large areas of gas and dust, including giant pillars that remain behind after intense radiation from massive stars has eroded the more diffuse gas.

A recent Chandra study of the cluster on the right side of the image, named NGC 2237, provides the first probe of the low-mass stars in this satellite cluster. Previously only 36 young stars had been discovered in NGC 2237, but the Chandra work has increased this sample to about 160 stars.

The presence of several X-ray emitting stars around the pillars and the detection of an outflow -- commonly associated with very young stars -- originating from a dark area of the optical image indicates that star formation is continuing in NGC 2237.

By combining these results with earlier studies, the scientists conclude that the central cluster formed first, followed by expansion of the nebula, which triggered the formation of the two neighboring clusters, including NGC 2237.

This work was led by Junfeng Wang of the Harvard-Smithsonian Center for Astrophysics. The co-authors were Eric Feigelson, Leisa Townsley, Pat Broos and Gordon Garmire from Penn State University, Carlos Roman-Zuniga from the German-Spanish Astronomical Center in Spain, and Elizabeth Lada from the University of Florida.

Explore further: Image: Hubble sweeps a messy star factory

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User comments : 2

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omatumr
1 / 5 (1) Sep 08, 2010
Thanks for the beautiful picture.

It seems consistent with the idea that the birth and death of a stars may related, as if the collapsed core of the older star is the accretion site for the new one.

Again, thanks for the picture.

With kind regards,
Oliver K. Manuel
Sarai_RSA
not rated yet Sep 16, 2010
Beautiful. Would this mean that the formation of young stars is necessarily accompanied by further collapse of gas into other young stars?

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