Spectroscopic Study of the Cygnus Superbubble

Details Spectroscopic Study of the Cygnus Superbubble Spectroscopic Study of the Cygnus Superbubble

Jun 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998ap%26ss.263..197t&link_type=abstract

Astrophysics and Space Science, v. 263, Issue 1/4, p. 197-200 (1998).

Astronomy and Astrophysics

Astrophysics

Scientific paper

The Cygnus Superbubble is a ring-like structure asociated with atomic and molecular gas, dust and objects related to recent star forming activity. Its origin and nature has been interpreted both as a single structure originated in OB asociations or as an arrangement of unrelated objects. We present a high resolution spectroscopic study of this region designed to probe the velocity and density structure of the gas asociated with the Superbubble.

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