Abstract
As part of a larger program to study spatially resolved jet / interstellar medium interactions in nearby Seyfert galaxies, we have obtained high spatial resolution spectrographic observations of the central regions of M 51 and its extra-nuclear cloud (XNC, Ford et al. 1985), using STIS on-board the Hubble Space Telescope (HST). In this paper, we present very preliminary results from these observations.
Original language | English |
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Pages (from-to) | 315-316 |
Journal | Proceedings of the International Astronomical Union |
Volume | 2004 |
Issue number | IAUS222 |
DOIs | |
Publication status | Published - 1 Mar 2004 |