SpitzerObservations of the Dusty Warped Disk of Centaurus A
Author(s) -
Alice C. Quillen,
M. H. Brookes,
Jocelyn Keene,
Daniel Stern,
Charles Lawrence,
M. W. Werner
Publication year - 2006
Publication title -
the astrophysical journal
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 2.376
H-Index - 489
eISSN - 1538-4357
pISSN - 0004-637X
DOI - 10.1086/504418
Subject(s) - physics , astrophysics , centaurus a , galaxy , astronomy , thick disk , spectral energy distribution , parallelogram , active galactic nucleus , halo , hinge , classical mechanics
Spitzer mid-infrared images of the dusty warped disk in the galaxy CentaurusA show a parallelogram-shaped structure. We successfully model the observedmid-infrared morphology by integrating the light from an emitting, thin, andwarped disk, similar to that inferred from previous kinematic studies. Themodels with the best match to the morphology lack dust emission within theinner 0.1 to 0.8 kpc, suggesting that energetic processes near the nucleus havedisturbed the inner molecular disk, creating a gap in the molecular gasdistribution.Comment: submitted to Ap
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