Year: 2000
Type: article
Abstract: We report the discovery of gas inflow motions toward the active nucleus of the Circinus galaxy caused by the nonaxisymmetric potential of a nuclear gas bar. Evidence for dust associated with the bar comes from the HST /NICMOS H - K color map, whereas the streaming motions along the gas bar are seen in the velocity field of the H 2 S (1) (1-0) emission line. The gas bar is about 100 pc long with a visual extinction in excess of 10 mag. Indication for the gaseous nature of this bar comes from the lack of a stellar counterpart even in the K band, where the extinction is greatly reduced. We also use the NICMOS emission-line images (Paα, [Si VI], and [Fe II]) to study the innermost region of the ionization cones and the nuclear star-forming activity. We discuss the possible relationship of these components with the gaseous bar.
Source: The Astrophysical Journal
DOI: 10.1086/308444
Authors: R. Maiolino, A. Alonso‐Herrero, S. Anders, A. Quillen, M. J. Rieke, G. H. Rieke, L. E. Tacconi‐Garman
Language: English
Subfield: Astronomy and Astrophysics
Field: Physics and Astronomy
Domain: Physical Sciences
Open Access status: bronze
Awards: G433322167, G4508913497, G58316358, G6273510985
OpenAlex ID: W2043985151
