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DB01-42, DB00-58 & DB00-6:
Stars of Wonder, Stars of Infrared and X-ray Light

DB01-42, DB00-58 & DB00-6
Credit: X-ray: NASA/CXC/Northwestern U./C.Law & F.Yusef-Zadeh; Infrared: 2MASS/UMass/IPAC-Caltech/NASA/NSF
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This montage shows three clusters of bright, young stars in X-ray (blue) and infrared (green) light that lie in the direction of the center of the Galaxy. Like many stars in the disk of the Galaxy, they are difficult, if not impossible, to see with an optical telescope because of interstellar dust that blocks the visible light.

Chandra X-ray Image of Galactic Center
Infrared and X-ray data provide evidence for a large amount of dust and gas along the line of sight to the cluster, DB01-42. Invisible to optical telescopes, it is located near the Galactic Center, about 26,000 light years from Earth. Most of the stars in the image produce infrared radiation from their surfaces which have temperatures of several thousand degrees Celsius. The X-radiation from the two bright X-ray sources near the center of the cluster requires gas with temperatures of millions of degrees.

Animation: DB01-42 in context of the Milky Way Center
Such extremely hot gas may be due to the collision of stellar winds from two closely orbiting stars. The two bright X-ray sources in the image are likely close binary stars with high-speed stellar winds. The diffuse X-ray glow could be caused by the combined heating of gas in the cluster by winds from many stars.

The light from the stars in the two clusters, DB00-58 and DB00-6 show much less X-ray and infrared absorption. This lower absorption, which still blocks much of the visible light, indicates that these star clusters are not in the Galactic Center, but are foreground objects. The way in which the X-rays are produced in these clusters is likely to be similar to DB01-42.

Common Fast Facts for DB01-42, DB00-58 & DB00-6:
Category  Normal Stars & Star Clusters,
The Milky Way Galaxy
Constellation  Sagittarius
Color Code  Energy (X-ray: Blue; Infrared: Green)
Instrument  ACIS
Credit  X-ray: NASA/CXC/Northwestern U./C.Law & F.Yusef-Zadeh; Infrared: 2MASS/UMass/IPAC-Caltech/NASA/NSF
Reference  C. Law & F. Yusef-Zadeh, Astrophys. J. 611:858-870, 2004 August 20
Fast Facts for DB01-42:
Coordinates (J2000)  RA 17h 44m 52.50s | Dec -29º 40' 48”
Scale  4.2 arcmin per side
Observation Date  Two pointings on July 20, 2001
Observation Time  6 hours
Obs. IDs  merged: 2270; 2278
Distance Estimate  About 26,000 light years
Fast Facts for DB00-58:
Coordinates (J2000)  RA 17h 44m 59.90s | Dec -28º 51' 37”
Scale  2.8 arcmin per side
Observation Date  Two pointings on July 18, 2001
Observation Time  6 hours
Obs. IDs  merged: 2284; 2287
Distance Estimate  Significantly less than 26,000 light years
Fast Facts for DB00-6:
Coordinates (J2000)  RA 17h 47m 9.40s | Dec -28º 46' 26”
Scale  3.1 arcmin per side
Observation Date  July 17, 2001
Observation Time  3 hours
Obs. ID  merged: 2288
Distance Estimate  Significantly less than 26,000 light years
More Information on DB01-42, DB00-58 & DB00-6:
More Images of DB01-42, DB00-58 & DB00-6
DB01-42, DB00-58 & DB00-6 Animations
DB01-42, DB00-58 & DB00-6 Handout: html | pdf
Zoom in on DB01-42 (flash)
Powerpoint and PDF
Download image for your desktop
Related Chandra Images:
Photo Album: Quintuplet Cluster (28 Jul 04)
Photo Album: Galactic Center Radio Arc (09 Jan 02)
Photo Album: Galactic Center (Survey) (09 Jan 02)
Photo Album: Arches Cluster (06 Jun 01)
More Information on The Milky Way Galaxy:
X-ray Astronomy Field Guide: The Milky Way Galaxy
Questions and Answers: The Milky Way Galaxy
Chandra Images: The Milky Way Galaxy
More Information on Normal Stars & Star Clusters:
X-ray Astronomy Field Guide: Normal Stars
Questions and Answers: Normal Stars & Star Clusters
Chandra Images: Normal Stars & Star Clusters


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