Study of Two Galactic Center Star-Forming Regions: Sgr B and Sgr C

Details Study of Two Galactic Center Star-Forming Regions: Sgr B and Sgr C Study of Two Galactic Center Star-Forming Regions: Sgr B and Sgr C

Apr 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005xrrc.proce3.06l&link_type=abstract

"X-Ray and Radio Connections (eds. L.O. Sjouwerman and K.K Dyer) Published electronically by NRAO, http://www.aoc.nrao.edu/event

Physics

X-Ray, Radio, Massive Star Cluster Outflows

Scientific paper

A variety of observations have shown Sgr B (G0.6-0.1) to be one of the most spectacular star-forming regions in the Galaxy. Similarly, Sgr C (G359.4-0.1) is host to sites of star formation as well as a collection of unusual non-thermal radio filaments. Using Chandra, Very Large Array, and Nobeyama Radio Observatory observations, we study the correlations between radio continuum, CS(1--0) molecular line, and X-ray emission from these sources, with a focus on the distribution of the neutral iron 6.4 keV line emission. We examine the hypothesis that such emission is evidence of past flaring from Sgr A* and present an alternative model. We also study the distribution of X-ray and radio point sources throughout these regions.

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