Sensitive HI Spectra Through the Arms of the SMC

Details Sensitive HI Spectra Through the Arms of the SMC Sensitive HI Spectra Through the Arms of the SMC

Apr 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006atnf.prop..152m&link_type=abstract

ATNF proposal C1543, Semester: April, 2006

Computer Science

Mag Clouds, Atca

Scientific paper

We request two complete 12 hour synthesis cycles of (total of ~24 hours) on the ATCA be allocated to obtaining high spatial resolution and sensitive measurements of the HI in the Magellanic Bridge, towards two continuum objects. These resulting data will be of sufficient spatial and velocity resolution to combine with proposed UVES spectroscopic measurements to enable accurate and precise measurements of the relative Ca II K/HI abundance levels in three different parts of the SMC: through two unrelated locations in the 'transverse' arm of the SMC, and one sight line through the 'radial' arm. We will therefore be probing, for the first time, the abundance levels of the kinematically distinct and tidally-generated arms of the SMC.

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