Abstract
We present radial velocities for 33 stars in an optically obscured field toward the Galactic bulge at l=–1.14°, b=1.81°. The radial velocities are derived from spectra of the 2.3 µm CO bandhead that is prominent in late type giants. The heliocentric radial velocity and velocity dispersion are -75 ± 24 km s-1 and 127 ± 16 km s-1 respectively.
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© 1994 Springer Science+Business Media Dordrecht
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Blum, R., Carr, J., Depoy, D., Sellgren, K., Terndrup, D. (1994). Radial Velocities of M Giants at 300 PC Projected Radius from the Galactic Center. In: McLean, I.S. (eds) Infrared Astronomy with Arrays. Astrophysics and Space Science Library, vol 190. Springer, Dordrecht. https://doi.org/10.1007/978-94-011-1070-9_164
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DOI: https://doi.org/10.1007/978-94-011-1070-9_164
Publisher Name: Springer, Dordrecht
Print ISBN: 978-94-010-4466-0
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