Analysis Of Submillimeter Mopra And Herschel Observations Of The Galactic Center

Details Analysis Of Submillimeter Mopra And Herschel Observations Of The Galactic Center Analysis Of Submillimeter Mopra And Herschel Observations Of The Galactic Center

Jan 2012

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2012aas...21925203t&link_type=abstract

American Astronomical Society, AAS Meeting #219, #252.03

Astronomy and Astrophysics

Astronomy

Scientific paper

Observations of low-J transitions of CO, 13CO, CS, taken using the Mopra telescope, and of [CI], [CII], [NII], and high-J transitions of CO, taken with the HIFI instrument on Herschel, were used to model the behavior in Bania Clumps 1 and 2 in order to determine their contribution to hydrogen inflow to the galactic center. Modeling was done using Cloudy 10.00, as last described by Ferland et al. (1998). Relative line intensities were used to estimate hydrogen density and kinetic temperature in components of the clumps for fixed temperature and ultraviolet-irradiated conditions. While preparing the [CII] and [NII] data for modelling, an experimental HEB baseline removal technique based on matching reference spectra by first derivative was used.

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