New Very Large Array images of NH 3 (1, 1),(2, 2), and (3, 3) emission in the central 10 pc
of the Galaxy trace filamentary streams of gas, several of which appear to feed the …

We have used the BIMA array to image the Galactic center with a 19 pointing mosaic in HCN
(1–0), HCO+(1–0), and H 42 α emission with 5 km s-1 velocity resolution and 13′′� 4′…

… Although this result is in agreement with Coil & Ho (1999, … 1, 1) velocity-integrated emission
from McGary et al. (2001). After … 7 K for the excitation temperature (Coil & Ho 1999, 2000), we …

… Technologies [7] and the other is a system proposed by McGary [8], [9]. The detection system
is … using an array of search coils, where the coil diameter is mm and the array dimension is …

We have used the BIMA array to image the Galactic Center with a 19-pointing mosaic in
HCN(1-0), HCO+(1-0), and H 42-alpha emission with 5 km/s velocity resolution and 13'' x 4'' …

Mosaics of the central 10 pc made with the VLA show that NH 3 (1, 1),(2, 2) and (3, 3) trace
many filamentary streams of gas and giant molecular clouds (GMCs) near the Galactic Center …

… Although this result is in agreement with Coil & Ho (1999, … (1,1) velocity integrated emission
from McGary et al. (2001). After … of 7 K for the excitation temperature (Coil & Ho 1999, 2000), …

Modernization in space systems requires employment of new light-weight, high performance
composite materials that reduce bulk weight and increase structural integrity. This thesis …

Using the new 23 GHz receivers at the Very Large Array (VLA), we have detected NH 3 (6, 6)
emission (ν= 25.056025 GHz) from hot (> 150 K) molecular clouds in the central 10 pc of …

… the NH3(3,3) observations of McGary et al. (2001); the NH3 … to the “northern ridge” of McGary
et al. (2001). The variation … 2,2) to (1,1) line ratio map by McGary et al. (2001), which they …