NASA/IPAC EXTRAGALACTIC DATABASE
Date and Time of the Query: 2019-05-21 T21:54:39 PDT
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For refcode 1988A&A...203...28S:
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Copyright by European Southern Observatory (ESO). Reproduced by permission
1988A&A...203...28S H I observations of the massive spiral galaxy NGC 5635 R.P. Saglia, and R. Sancisi Scuola Normale Superiore, I-56100 Pisa, Italy Kapteyn Astronomical Institute, Postbus 800, NL-9700 AV Groningen, The Netherlands Received February 15, accepted March 29, 1988 Summary. H I observations of the S pec galaxy NGC 5635 with the Westerbork Synthesis Radio Telescope are presented. The large values of its mass and mass/luminosity ratio (7.5 10^11^ M_sun_ and 28 M_sun_/L_sun_ inside R_25_ = 22 kpc) and the strong asymmetries in the light and the hydrogen distributions are the most prominent characteristics of this spiral galaxy. NGC 5635 and other massive disk galaxies seem to be somewhat displaced from the Tully-Fisher relation towards larger velocities and lower luminosities. Two companion galaxies, an edge-on spiral and a dwarf irregular, were also detected in H I. Key words: spiral galaxies - kinematics and dynamics of galaxies - radio 21 cm-line
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