Opening A Window On [CII] And [NII] Emission In The Milky Way: HIGGS And STO

Details Opening A Window On [CII] And [NII] Emission In The Milky Way: HIGGS And STO Opening A Window On [CII] And [NII] Emission In The Milky Way: HIGGS And STO

May 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009aas...21442002m&link_type=abstract

American Astronomical Society, AAS Meeting #214, #420.02; Bulletin of the American Astronomical Society, Vol. 41, p.690

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Scientific paper

The Stratospheric Terahertz Observatory (STO) is a soon to be flown long duration balloon experiment to measure [NII] and [CII] over a broad area of the galactic plane. While the Herschel Inner Galaxy Gas Survey (HIGGS) is an approved Herschel Key Project to use the HIFI and PACS instruments to observe [CII], [NII], [OI], [OIII], and high-J CO emission lines in focussed regions near the Galactic Center. Using a combination of the data from these two projects we plan to open a window into the dynamics of molecular clouds that can be used as a template for other galaxies observable with ALMA. We'll discuss the data that both of these projects will collect along with the synergies between them.

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