Images by Date
Images by Category
Solar System
Stars
White Dwarfs
Supernovas
Neutron Stars
Black Holes
Milky Way Galaxy
Normal Galaxies
Quasars
Galaxy Clusters
Cosmology/Deep Field
Miscellaneous
Images by Interest
Space Scoop for Kids
Multiwavelength
Sky Map
Constellations
3D Wall
Photo Blog
Top Rated Images
Image Handouts
Desktops
High Res Prints
Fits Files
Image Tutorials
Photo Album Tutorial
False Color
Cosmic Distance
Look-Back Time
Scale & Distance
Angular Measurement
Images & Processing
AVM/Metadata
Getting Hard Copies
Image Use Policy
Web Shortcuts
Chandra Blog
RSS Feed
Chandra Mobile
Chronicle
Email Newsletter
News & Noteworthy
Image Use Policy
Questions & Answers
Glossary of Terms
Download Guide
Get Adobe Reader
More Information
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
Related Podcasts
A Tour of Eta Carinae
Download Image

More Information
Handout
Handout: html | pdf

More Images
Chandra X-ray Image
of W3 Main
(Credit: NASA/CXC/Penn State/L.Townsley et al.)


Related Images
NGC 3576
NGC 3576
(26 Sep 06)
Trumpler 14
Trumpler 14
(31 Aug 05)
M17
M17
(14 Aug 03)
W3 Main:
A Productive Star Formation Factory


W3 Main
Credit: X-ray: NASA/CXC/Penn State/L.Townsley et al.; Optical: Pal Obs. DSS

W3 is a region where many massive stars are forming in a string of stellar clusters, located about 6,000 light years from Earth in the Perseus arm of the Milky Way galaxy. W3 is part of a vast molecular cloud complex that also contains the W4 superbubble (not seen in this image). Scientists believe that the extraordinary amount of star formation in W3 has possibly been influenced by neighboring W4, an inflating bubble of gas over 100 light years across. W4 may directly trigger the birth of W3's massive stellar clusters as it expands and sweeps up molecular gas into a high-density layer at its edge, within which stars can form. Another possible scenario is that W4's expansion has caused a domino effect of star formation, forming the cluster IC 1795 (seen as a clump of X-ray sources in the bottom left corner of this image) which in turn triggered formation of the young, massive clusters in W3.

In this composite image of one of the many star-forming complexes of W3, called W3 Main, green and blue represent lower and higher-energy X-rays, respectively, while red shows optical emission. Hundreds of X-ray sources are revealed in this central region of W3 Main. These bright point-like objects are an extensive population of several hundred young stars, many of which were not found in earlier infrared studies. These Chandra data show that W3 Main is the dominant star formation region of W3. Because its X-ray sources are all at the same distance, yet span a range of masses, ages, and other properties, W3 is an ideal laboratory for understanding recent and ongoing star formation in one of the Milky Way's spiral arms.

Fast Facts for W3 Main:
Credit  X-ray: NASA/CXC/Penn State/L.Townsley et al.; Optical: Pal Obs. DSS
Scale  Image is 14 arcmin across
Category  Normal Stars & Star Clusters
Coordinates (J2000)  RA 02h 25m 40.60s | Dec +62 05' 52.40"
Constellation  Cassiopeia
Observation Dates  23 Mar 00, 03 Apr 00, 04 Jan 05
Observation Time  22 hours
Obs. IDs  611, 446, 5890
Color Code  Energy (X-ray: Blue & Green; Optical: Red;)
Instrument  ACIS
Distance Estimate  About 6,000 light years
Release Date  December 18, 2006