Chandra X-ray Observatory - HomeAbout The ChandraEducational MaterialsField GuidePhoto AlbumPress RoomResources
Chandra X-ray Observatory - HomeChandra Photo Album - You are here
ObservatoryImages by DateImages by CategorySky MapConstellationsSpecial FeaturesChandra Zoom-insImage HandoutsScale Bar ImagesTutorial Chandra Images & False Color Note on Cosmic DistanceCosmic Look Back TimeScale & DistanceScale & Angular MeasurementImage Use
Web Site ToolsVisit the Chandra ChroniclesEmail NewsletterSite MapNew & NoteworthyImage Use PolicyQuestions & AnswersGlossaryDownload Guide

More Images of M83

Click for large jpg
Chandra Close-up of M83 Nucleus
Chandra's close-up of M83 shows a bright nuclear region glowing prominently due to a cloud of hot gas and a high concentration of neutron stars and black holes that were created during a burst of star formation that is estimated to have begun about 20 million years ago in the galaxy's time frame.
Scale: Image is 3 arcmin on a side
(Credit: NASA/CXC/U.Leicester/U.London/R.Soria & K.Wu)

Click for large jpg
Chandra & VLT Image of M83
The red dots on this image represent X-ray point sources detected by Chandra in M83. The X-ray sources are overlaid on an optical image of the spiral galaxy obtained with ESO's Very Large Telescope in Chile.
Scale: Image is 6.8 arcmin on a side
(Credit: NASA/CXC/U.Leicester/U.London/R.Soria & K.Wu)

Click for large jpg
VLA Radio image of M83
(Credit: C.Stockdale (NRL/NRC), J.Cowan, L.Maddox (Univ. of Oklahoma), & M. Rupen (NRAO/AUI/NSF))

Click for large jpg
HST Image of M83 Central Region
This HST image reveals that there is active star formation in both the bright nucleus of M83 as well as farther out in the spiral arms where bluer stars are seen. In between the nucleus and the outer spiral arms, there is a greenish-colored, bar-shaped region. Astronomers believe this area contains middle-aged stars and that it is largely devoid of active star formation.
(Credit: NASA/HST)

Click for large jpg
HST Close-up of M83 Nucleus
This HST image reveals that there is active star formation in both the bright nucleus of M83 as well as farther out in the spiral arms where bluer stars are seen. In between the nucleus and the outer spiral arms, there is a greenish-colored, bar-shaped region. Astronomers believe this area contains middle-aged stars and that it is largely devoid of active star formation.
(Credit: NASA/HST)


Return to M83 (22 Jan 03)

Chandra Images: '08 | ' 07 | ' 06 | ' 05 | ' 04 | ' 03 | ' 02 | ' 01 | ' 00 | ' 99 | Images by Category




separator line
CXC Home | Search | Help | Site Map | Image Use Policy | Privacy & Accessibility | Downloads & Plugins
Latest Images | New & Noteworthy | Multimedia | Flash Ecards | Glossary | Q&A | Guestbook


RSS Feed RSS Feed | Podcast Podcast | Blog Blog

[News by email: Chandra Digest]
[Contact us: cxcpub@cfa.harvard.edu]
NASA's Home Page Smithsonian's Home Page CXC Home Page Image Map for NASA's, Smithsonian and Chandra's Home Pages
Harvard-Smithsonian Center for Astrophysics
60 Garden Street, Cambridge, MA 02138 USA
Phone: 617.496.7941 Fax: 617.495.7356


Text Size:
normal font large font larger font
Chandra X-ray Center, Operated for NASA by the Smithsonian Astrophysical Observatory
This site was developed with funding from NASA under Contract NAS8-03060.
Revised: April 09, 2007