Credit: X-ray (NASA/CXC/SAO/J. Wang et al),
Optical (DSS & NOAO/AURA/NSF/KPNO 0.9-m/T. Rector et al)
This composite image shows the Rosette star formation region, located about 5,000 light years from Earth. Data from the Chandra X-ray Observatory are colored red and outlined by a white line (roll your mouse over the image above). The X-rays reveal hundreds of young stars in the central cluster and fainter clusters on either side. Optical data from the Digitized Sky Survey 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.
Fast Facts for Rosette Nebula:
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.
Fast Facts for Rosette Nebula:
Scale: Image is 1 degree across (about 87 light years).
Category: Normal Stars & Star Clusters
Coordinates (J2000) RA 06h 31m 52.00s Dec +04° 55' 57.00"
Constellation: Monoceros
Observation Date: 4 pointings on 5-6 Jan 2001, 1 Jan 2004, 9 Feb 2007
Observation Time: 50 hours (2 days 2 hours)
Obs. ID: 1874-1877, 3750, 8454
Color Code: Optical (Purple, Orange, Green, Blue); X-ray (Red)
Instrument: ACIS
References: Wang et al, 2010 ApJ 716:474-489
Distance Estimate: About 5,000 light years
Category: Normal Stars & Star Clusters
Coordinates (J2000) RA 06h 31m 52.00s Dec +04° 55' 57.00"
Constellation: Monoceros
Observation Date: 4 pointings on 5-6 Jan 2001, 1 Jan 2004, 9 Feb 2007
Observation Time: 50 hours (2 days 2 hours)
Obs. ID: 1874-1877, 3750, 8454
Color Code: Optical (Purple, Orange, Green, Blue); X-ray (Red)
Instrument: ACIS
References: Wang et al, 2010 ApJ 716:474-489
Distance Estimate: About 5,000 light years
