Shells, Bubbles, and Chimneys in the Southern Galactic Plane Survey

Details Shells, Bubbles, and Chimneys in the Southern Galactic Plane Survey Shells, Bubbles, and Chimneys in the Southern Galactic Plane Survey

Jan 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003rmxac..15..287m&link_type=abstract

Winds, Bubbles, and Explosions: a conference to honor John Dyson, Pátzcuaro, Michoacán, México, September 9-13, 2002 (Eds. S. J.

Astronomy and Astrophysics

Astronomy

Ism: Bubbles, Ism: Structure

Scientific paper

The H I Southern Galactic Plane Survey (SGPS) is an ideal dataset with which to explore the impact of massive stars on the Galactic ISM. We are using the SGPS to study the global properties of H I shells over size scales ranging from tens of parsecs to kiloparsecs. Here we present an intriguing Galactic chimney and discuss the Galactic distribution of large H I shells with respect to Galactic radius and spiral arms.

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