KECK SPECTROSCOPY OF DWARF ELLIPTICAL GALAXIES IN THE VIRGO CLUSTER
Marla Geha, Puragra Guhathakurta, Roeland P. van der Marel
Abstract
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Marla Geha, Puragra Guhathakurta, Roeland P. van der Marel
Abstract
Open-access reader
Keck spectroscopy is presented for four dwarf elliptical galaxies in the Virgo Cluster. At this distance, the mean velocity and velocity dispersion are well resolved as a function of radius between 100 to 1000 pc, allowing a clear separation between nuclear and surrounding galaxy light. We find a variety of dispersion profiles for the inner regions of these objects, and show that none of these galaxies is rotationally flattened. 1
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Keck spectroscopy is presented for four dwarf elliptical galaxies in the Virgo Cluster. At this distance, the mean velocity and velocity dispersion are well resolved as a function of radius between 100 to 1000 pc, allowing a clear separation between nuclear and surrounding galaxy light. We find a variety of dispersion profiles for the inner regions of these objects, and show that none of these galaxies is rotationally flattened. 1
Key concepts: Virgo Cluster, Dwarf galaxy, Spectroscopy, Astronomy, Physics, Astrophysics, Cluster (spacecraft), Galaxy cluster