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The central regions of M 51 observed with HST/STIS

Published online by Cambridge University Press:  01 December 2004

P. Ferruit
Affiliation:
CRAL-Observatoire de Lyon, 9 avenue Charles André, 69561 Saint Genis Laval cedex, France
L. D. Bradley
Affiliation:
Department of Physics and Astronomy, The John Hopkins University, 3400 N. Charles Street, Baltimore, MD 21218, USA
M. E. Kaiser
Affiliation:
Department of Physics and Astronomy, The John Hopkins University, 3400 N. Charles Street, Baltimore, MD 21218, USA
G. Cecil
Affiliation:
Department of Physics and Astronomy, CB3255, University of North Carolina, Chapel Hill, NC 27599, USA
C. G. Mundell
Affiliation:
Astrophysics Research Institute, Liverpool John Moores University, Twelve Quays House, Egerton Wharf, Birkenhead CH41 1LD, UK
B. Jungwiert
Affiliation:
CRAL-Observatoire de Lyon, 9 avenue Charles André, 69561 Saint Genis Laval cedex, France
E. Emsellem
Affiliation:
CRAL-Observatoire de Lyon, 9 avenue Charles André, 69561 Saint Genis Laval cedex, France
A. S. Wilson
Affiliation:
Astronomy Department, University of Maryland, College Park, MD 20742, USA
Y. Terashima
Affiliation:
Institute of Space and Astronautical Science, 3-1-1 Yoshinodai, Sagamihara, Kanagawa, 229-8510, Japan
L. Binette
Affiliation:
Instituto de Astronomia, UNAM, Apdo. 70-264, 04510 D. F., Mexico
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Abstract

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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.To search for other articles by the author(s) go to: http://adsabs.harvard.edu/abstract_service.html

Type
POSTERS
Copyright
© 2004 International Astronomical Union

Footnotes

Based on observations with the NASA/ESA Hubble Space Telescope obtained at the Space Telescope Science Institute, which is operated by the Association of Universities for Research in Astronomy, Inc., under NASA contract NAS 5-26555