New Insights Into The X-ray Properties Of NGC 1672

Details New Insights Into The X-ray Properties Of NGC 1672 New Insights Into The X-ray Properties Of NGC 1672

Sep 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006head....9.1306j&link_type=abstract

American Astronomical Society, HEAD meeting #9, #13.06; Bulletin of the American Astronomical Society, Vol. 38, p.367

Astronomy and Astrophysics

Astronomy

Scientific paper

We present the first results of new Chandra and XMM-Newton X-ray observations of the barred spiral galaxy NGC1672. Previously classified as a Seyfert galaxy, the new combined X-ray imaging and spectral information provides evidence that the nucleus of the galaxy may be almost entirely starburst in nature, presumably triggered and sustained by gas and dust driven to the central region along the galactic bar.

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