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Normal Stars & Star Clusters
X-ray Astronomy Field Guide
Normal Stars & Star Clusters
Questions and Answers
Normal Stars & Star Clusters
Chandra Images
Normal Stars & Star Clusters
Animations & Video: Normal Stars & Star Clusters
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Click for high-resolution animation
1. Into the Milky Way: Quintuplet Cluster
QuicktimeMPEG This sequence begins with Chandra's X-ray view of a 900 by 400 light year swath of the center of the Milky Way. It then zooms into a smaller region where large filamentary structures are seen in radio waves. The view moves in even closer to show the Quintuplet star cluster. Named for its five brightest stars at infrared wavelengths, the Quintuplet is known to be home to hundreds of stars. Several of these are very massive stars that are rapidly losing gas from their surfaces in high-speed stellar winds. Collisions from these winds are what astronomers believe to be the source for the point-like concentrations seen in the Chandra image.
[Runtime: 0:24]
(X-ray: NASA/CXC/NWU/C.Law & F.Zadeh; IR: NASA/ESO/STScI/D.Figer et al.; Radio: NRAO/AUI/NSF/F.Zadeh et al.)

Related Chandra Images:

Click for high-resolution animation
2. Towards the Milky Way: DB00-6
QuicktimeMPEG his series of images shows the DB00-58 star cluster in context with Chandra's 900- by 400-light year mosaic of the Galactic Center. The view then transitions to radio emission from a smaller region that includes DB00-6, before showing infrared data, and ending with Chandra's X-ray close-up. . Despite DB00-6's similar appearance to DB01-42 (#1, above), the X-ray and infrared information show that DB00-6 is, in fact, a foreground object, and is significantly closer to us than 25,000 light years.
[Runtime: 0:24]
(X-ray: NASA/CXC/Northwestern U./C.Law & F.Yusef-Zadeh; Infrared: 2MASS/UMass/IPAC-Caltech/NASA/NSF; Radio: NRAO/AUI/NSF/F.Zadeh et al.)

Related Chandra Images:

Click for high-resolution animation
3. Towards the Milky Way: DB00-58
QuicktimeMPEG This series of images shows the DB00-58 star cluster in context with Chandra's 900- by 400-light year mosaic of the Galactic Center. The view then transitions to infrared emission from a smaller region that includes DB00-58, before showing Chandra's X-ray close-up. Despite DB00-58's similar appearance to DB01-42 (#1, above), the X-ray and infrared information show that DB00-58 is, in fact, a foreground object, and is significantly closer to us than 26,000 light years.
[Runtime: 0:20]
(X-ray: NASA/CXC/Northwestern U./C.Law & F.Yusef-Zadeh; Infrared: 2MASS/UMass/IPAC-Caltech/NASA/NSF)

Related Chandra Images:

Click for high-resolution animation
4. DB01-42 in context of the Milky Way Center
QuicktimeMPEG This series of images puts the cluster known as DB01-42 in context with Chandra's 900- by 400-light year mosaic of the Galactic Center. The view then transitions to radio emission from a smaller region that includes DB01-42, before showing infrared data of the same area, and ending with Chandra's X-ray close-up. Chandra's X-ray data have helped astronomers identify DB01-42 as a member of the Galactic Center. It is about 26,000 light years away from Earth.
[Runtime: 0:10]
(X-ray: NASA/CXC/Northwestern U./C.Law & F.Yusef-Zadeh; Infrared: 2MASS/UMass/IPAC-Caltech/NASA/NSF; Radio: NRAO/AUI/NSF/F.Zadeh et al.)

Related Chandra Images:

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