Observations of CO in the eastern filaments of NGC 1275
P. Salom\'e, Y. Revaz, F. Combes, J. Pety, D. Downes, A.C. Edge, and, A.C. Fabian

TL;DR
This study presents high-resolution CO(2-1) interferometer maps of the eastern filaments around NGC 1275, revealing cold molecular clouds with narrow lines, likely falling back into the galaxy, supporting models of AGN-driven positive feedback.
Contribution
First high-resolution CO(2-1) interferometer observations of NGC 1275's eastern filaments, revealing unresolved molecular cloud structures and their potential role in galaxy feedback processes.
Findings
Detection of CO emission along 5 kpc filaments
Identification of narrow line-width (~30 km/s) molecular clouds
Evidence supporting self-gravitating, falling molecular clouds in galaxy feedback
Abstract
We recently found extended CO(2-1) emission from cold molecular gas embedded in the network of Halpha filaments surrounding the galaxy NGC 1275 (Salome et al. 2006). We now present CO(2-1) interferometer maps of the eastern filaments, at high spatial and spectral resolutions. The cold molecular gas is detected by the Plateau de Bure Interferometer along the eastern filaments over an extent of 15'', or with a projected length of 5kpc. In our 2.5'' beam, the main CO filament is mostly unresolved along its minor axis. The multiple peaks along the CO filaments and the low values of the observed CO brightness temperatures imply further unresolved structures that may be giant molecular clouds. These clouds have very narrow line-width emission lines (~30 km/s). The CO emission is optically thick. It very likely traces cold clouds bound under their own self-gravity that may be falling back in…
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