Large stellar disks in small elliptical galaxies

Details Large stellar disks in small elliptical galaxies Large stellar disks in small elliptical galaxies

1999-03-02

arxiv.org/abs/astro-ph/9903040v1

Astrophys.J. 513 (1999) L25

Astronomy and Astrophysics

Astrophysics

11 pages LaTex with 4 Postscript figures

Scientific paper

10.1086/311894

We present the rotation velocities V and velocity dispersions sigma along the principal axes of seven elliptical galaxies less luminous than M_B= -19.5. These kinematics extend beyond the half-light radii for all systems in this photometrically selected sample. At large radii the kinematics not only confirm that rotation and "diskiness" are important in faint ellipticals, as was previously known, but also demonstrate that in most sample galaxies the stars at large galactocentric distances have (V/sigma)_max of about 2, similar to the disks in bona-fide S0 galaxies. Comparing this high degree of ordered stellar motion in all sample galaxies with numerical simulations of dissipationless mergers argues against mergers with mass ratios <=3:1 as an important mechanism in the final shaping of low-luminosity ellipticals, and favors instead the dissipative formation of a disk.

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