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Title:
Mid-infrared properties of Arp102B
Authors:
Devore, H.; Chary, R.-R.; Chapple, L.; Chun, H.; Mills, K.; Graves, B.; Kerr, C.; Cordoza, B.
Affiliation:
AA(Cape Fear High School, Fayetteville, NC), AB(Spitzer Science Center, Caltech, Pasadena, CA), AC(Traverse City East Junior High School, Traverse City, MI), AD(Cranston High School, East Cranston, RI), AE(Cape Fear High School, Fayetteville, NC), AF(Cape Fear High School, Fayetteville, NC), AG(Cranston High School, East Cranston, RI), AH(Cranston High School, East Cranston, RI)
Publication:
American Astronomical Society Meeting 207, #140.10; Bulletin of the American Astronomical Society, Vol. 37, p.1396
Publication Date:
12/2005
Origin:
AAS
Bibliographic Code:
2005AAS...20714010D

Abstract

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 Mȯ . 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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