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Kinematics and Warp in NGC 4565

Published online by Cambridge University Press:  04 August 2017

S. Casertano ,
R. Sancisi  and
T. S. van Albada
S. Casertano
Affiliation:
Institute for Advanced Study, Princeton, NJ 08540 - USA
R. Sancisi
Affiliation:
Kapteyn Laboratorium, Postbus 800, 9700 AV Groningen - The Netherlands
T. S. van Albada
Affiliation:
Kapteyn Laboratorium, Postbus 800, 9700 AV Groningen - The Netherlands

Abstract

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We present preliminary results of the analysis of WSRT observations of the edge-on spiral NGC 4565 (Sancisi 1985). The neutral hydrogen layer of this galaxy extends to 1.3 R25, permitting to trace the rotation curve outside the optical edge of the system, and is warped in the outer parts.

Type
Research Article
Information
Symposium - International Astronomical Union , Volume 117: Dark Matter in the Universe , 1987 , pp. 82
Copyright
Copyright © Reidel 1987 

References

Sancisi, 1985, in preparation.Google Scholar
van der Kruit, P. C. and Searle, L. 1981, Astr. Ap., 95, 105.Google Scholar