Astronomy Picture of the Day

Explanation: Our Galaxy is filled with gas. Most of this gas is hydrogen, some is helium, but there is a trace amount of relatively heavy molecules, including carbon monoxide (CO) - a component of smog. The above wide-angle radio CO image shows the incredibly diverse structures that the molecular interstellar medium forms. Dense clouds show where stars may be forming and open voids may indicate the action of strong winds from massive, recently formed stars. This FCRAO Outer Galaxy Survey was recently re-processed at the Dominion Radio Astrophysical Observatory for inclusion in the Canadian Galactic Plane Survey, an international effort to map all constituents of the interstellar medium over large scales at high angular resolution.

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Authors & editors: Robert Nemiroff (MTU) & Jerry Bonnell (USRA)
NASA Web Site Statements, Warnings, and Disclaimers
NASA Official: Jay Norris. Specific rights apply.
A service of: LHEA at NASA / GSFC
& Michigan Tech. U.

Publications with keywords: CO2 - interstellar medium - outer Galaxy
Publications with words: CO2 - interstellar medium - outer Galaxy
See also:

• Mountains of Creation
• A Sky Full Of Hydrogen
• Fractal Interstellar Dust Up Close
• The Local Bubble and the Galactic Neighborhood
• The Local Interstellar Cloud
• The Solar Neighborhood