M33 in radio and optical

Image courtesy of NRAO/AUI · Download full size image

This image of the Triangulum Galaxy was created by combining optical data from the National Science Foundation's 0.9-meter telescope on Kitt Peak in Arizona with radio data from the National Science Foundation's Very Large Array (VLA) telescope in New Mexico and the Westerbork Synthesis Radio Telescope (WSRT) in the Netherlands. Also known as M33, the Triangulum Galaxy is part of the Local Group of galaxies, which includes the Andromeda Galaxy (M31) and our galaxy, the Milky Way. M33 is over thirty thousand light years across, and more than two million light years away.

The optical data in this image show the many stars within the galaxy as well as reddish star forming regions that are filled with hot Hydrogen gas. The radio data reveal the cool Hydrogen gas within the galaxy, gas which cannot be seen with an optical telescope. Combined together, the radio and optical give a more comprehensive view of star formation in this galaxy. The color image was generated by combining images Posted on: 04 Nov, 2003

• Hubble Space Telescope
• Chandra X-ray Observatory
• Compton Gamma-Ray Observatory
• ROSAT X-ray Observatory
• SOHO Solar Observatory
• WMAP
• 2MASS Sky Survey
• ASTER Earth Imaging Instrument
• MISR Earth Imaging Instrument
• NRAO Gallery
• NAOJ Subaru Telescope
• Galaxy Evolution Explorer (GALEX)
• European Southern Observatory (ESO)
• Wide-Field Imager (WFI)
• SOFI Infrared Multi-mode Instrument
• Canada-France-Hawaii Telescope (CFHT)
• New Technology Telescope (NTT)
• Atacama Pathfinder Experiment (APEX)
• SOHO Daily Images - 1996
• Spitzer Space Telescope (SIRTF)
• Infrared Legacy Gallery

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