Spectropolarimetric Test of the Relativistic Disk Model for the Broad H alpha Line of ARP 102B

Details Spectropolarimetric Test of the Relativistic Disk Model for the Broad H alpha Line of ARP 102B Spectropolarimetric Test of the Relativistic Disk Model for the Broad H alpha Line of ARP 102B

Jan 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996apj...456l..25a&link_type=abstract

Astrophysical Journal Letters v.456, p.L25

Astronomy and Astrophysics

Astronomy

23

Galaxies: Active, Galaxies: Individual Name: Arp 102B, Galaxies: Nuclei, Galaxies: Seyfert, Accretion, Accretion Disks

Scientific paper

The favored form of the relativistic disk model for the broad H alpha
line of Arp 102B leads to predictions for the percent polarization,
polarized flux profile, and polarization position angle of the line. The
line is polarized, but observations do not confirm the specific
predictions.

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