The Herschel Inner Galaxy Gas Survey (HIGGS): Early Results

Details The Herschel Inner Galaxy Gas Survey (HIGGS): Early Results The Herschel Inner Galaxy Gas Survey (HIGGS): Early Results

May 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010aas...21641205m&link_type=abstract

American Astronomical Society, AAS Meeting #216, #412.05; Bulletin of the American Astronomical Society, Vol. 41, p.822

Astronomy and Astrophysics

Astronomy

Scientific paper

The Herschel Inner Galaxy Gas Survey (HIGGS) is a Herschel Open Time Key Programme to use the HIFI and PACS instruments to observe [CII], [NII], [OI], [OIII], and high-J CO emission lines in focused regions near the Galactic Center. By separating and evaluating the distinctly different roles of the central nuclear engine, the Galactic Bar, and dynamical stellar and interstellar feedback mechanisms, HIGGS will provide a high-resolution template for the physical processes in galactic nuclei throughout the local universe, in particular those engaged in starburst activity.
We intend to present our early results along with a description of the data reduction and analysis tools that we have developed.

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