An Orbit Fit for the Grillmair Dionatos Cold Stellar Stream

Abstract

We use velocity and metallicity information from SDSS and SEGUE stellar spectroscopy to fit an orbit to the narrow $63^{\circ }$ stellar stream of Grillmair and Dionatos. The stars in the stream have a retrograde orbit with eccentricity $e=0.33$ (perigalacticon of 14.4 kpc and apogalacticon of 28.7 kpc) and inclination approximately $i\sim 35^{\circ }$. In the region of the orbit which is detected, it has a distance of about 7 to 11 kpc from the Sun. Assuming a standard disk plus bulge and logarithmic halo potential for the Milky Way stars plus dark matter, the stream stars are moving with a large space velocity of approximately $276\mathrm{km}{\mathrm{s}}^{-1}$ at perigalacticon. Using this stream alone, we are unable to determine if the dark matter halo is oblate or prolate. The metallicity of the stream is [Fe/H] $=-2.1\pm 0.1$. Observed proper motions for individual stream members above the main sequence turnoff are consistent with the derived orbit. None of the known globular clusters in the Milky Way have positions, radial velocities, and metallicities that are consistent with being the progenitor of the GD-1 stream.

44 pages, 4 tables, 14 figures. Accepted for publication into Astrophysical Journal

References in corpus (5)

• The SEGUE Stellar Parameter Pipeline. I. Description and Initial Validation Tests
• The SEGUE Stellar Parameter Pipeline. II. Validation with Galactic Globular and Open Clusters
• The SEGUE Stellar Parameter Pipeline. III. Comparison with High-Resolution Spectroscopy of SDSS/SEGUE Field Stars
• Discovery of a Giant Stellar Tidal Stream Around the Disk Galaxy NGC 4013
• Fiducial Stellar Population Sequences for the u'g'r'i'z' System

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