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Abundances and kinematics of K giants in the galactic nuclear bulge

Thesis/Dissertation ·
OSTI ID:6696424
Spectroscopy and photometry were obtained for 100 K giants in Baade's Window at l = 1/sup 0/, b = -4/sup 0/. The abundance distribution of the nuclear bulge K giants was derived relative to 45 stars of known abundance. The abundances run from -1 to nearly +1 dex, with a peak at 0.3 dex, or twice the solar abundance. Of the 88 stars with derived abundances, 22% exceeded the abundance of the most metal rich local K giants; 50% exceeded the solar abundance, and 10% were metal poor (< -0.6 dex). Radial velocities were measured for 53 nuclear bulge K giants which also have derived abundances. Their velocity dispersion is 104 km/sec. The mean velocity is -19 +/- 14 km/sec; within 1 sigma of the solar Pi velocity of -10 km/sec. When this sample is divided into 3 subsets based on the abundances, the subset of 21 stars > 0.3 dex has sigma = 92 +/- 14 km/sec and the metal poor subset of 16 stars <-0.3 dex has J = 126 +/- 22 km/sec. An intermediate set of 16 stars has sigma = 97 +/- 17 km/sec. The most metal rich stars may have a bulk velocity of -38 +/- 14 km/sec, 1sigma less than the -19 km/sec of the metal poor stars. No evidence was found that either the metal rich or metal poor stars follow the galactic rotation curve; hence, neither population appears to be rotation supported. Optical and infrared photometry is presented for nuclear bulge K giants. The colors of these stars are shown to be too hot for their derived metal abundances.
Research Organization:
California Inst. of Tech., Pasadena (USA)
OSTI ID:
6696424
Country of Publication:
United States
Language:
English