Mid-infrared properties of Arp102B

Details Mid-infrared properties of Arp102B Mid-infrared properties of Arp102B

Dec 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005aas...20714010d&link_type=abstract

American Astronomical Society Meeting 207, #140.10; Bulletin of the American Astronomical Society, Vol. 37, p.1396

Astronomy and Astrophysics

Astronomy

Scientific paper

Arp 102B is a subluminous, radio-loud LINER1.8 galaxy at z=0.024. It is thought to harbor a nuclear black hole, estimated to be ˜108 M&sun; . We present sub-arcsec imaging of the nucleus between 10-20 μ m from Keck and R ˜60-600 spectroscopy between 5-40 μ m with the Spitzer/IRS. We use the data to place constraints on the bolometric luminosity, dust temperature, nature of dust and physical conditions of the line emitting gas in the vicinity of the supermassive black hole.

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