1990Monthly Notices of the Royal Astronomical SocietyOpen access

Mass decomposition of spiral galaxies from disc kinematics

MASSIMO PERSIC, P. Salucci

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Abstract

Summary We devise a method for the disc/halo mass decomposition of the rotation curves of spiral galaxies that was outlined by us in a previous paper. Upon application to a larger sample of 58 spirals, we confirm our earlier results. In particular, we find that the disc-to-halo mass ratio at the optical radius, Mdisc/Mhalo, is a strong function of luminosity, Mdisc/Mhalo α LB2/3.

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Summary We devise a method for the disc/halo mass decomposition of the rotation curves of spiral galaxies that was outlined by us in a previous paper. Upon application to a larger sample of 58 spirals, we confirm our earlier results. In particular, we find that the disc-to-halo mass ratio at the optical radius, Mdisc/Mhalo, is a strong function of luminosity, Mdisc/Mhalo α LB2/3.

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Available abstract

Summary We devise a method for the disc/halo mass decomposition of the rotation curves of spiral galaxies that was outlined by us in a previous paper. Upon application to a larger sample of 58 spirals, we confirm our earlier results. In particular, we find that the disc-to-halo mass ratio at the optical radius, Mdisc/Mhalo, is a strong function of luminosity, Mdisc/Mhalo α LB2/3.

Key concepts: Physics, Galaxy rotation curve, Spiral galaxy, Astrophysics, Halo, Disc galaxy, Spiral (railway), Galaxy

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Mass decomposition of spiral galaxies from disc kinematics — Research Paper | ScholarLens