Probing Relativistic Outflows in Extreme NLS1

Details Probing Relativistic Outflows in Extreme NLS1 Probing Relativistic Outflows in Extreme NLS1

Sep 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999cxo..prop...42n&link_type=abstract

Chandra Proposal ID #01700358

Physics

Chandra Proposal Id #01700358

Scientific paper

The most extreme objects in the class of ``Narrow-Line'' Seyfert 1 galaxies (NLS1) show absorption features which are probably due to oxygen in a relativistic wind outflowing from the nucleus. The features are blueshifted to 1-1.5 keV and therefore occur close to the peak efficiency of the MEG. We propose to use that instrument to confirm the features and measure their energy, strength and profiles to probe this unusual relativistic flow, which may represent an analogue of the BAL phenomenon observed in the UV.

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