A CS J = 5 -> 4 Mapping Survey Towards High Mass Star Forming Cores Associated with H2O Masers
In this survey we have systematically mapped 63 cloud cores in the CS J = 5 -> 4 line towards
7 indexed results
In this survey we have systematically mapped 63 cloud cores in the CS J = 5 -> 4 line towards
With a study of bulk GaAs and GaP, we report detailed infrared spectra and their temperature dependence from first principles.
We have compared the intensity distribution of molecular line emission with that of dust continuum emission, and modeled molecular line
Twenty-four cores have been mapped in CS J = 7 -> 6 at the CSO. From the spectra we determine
We have observed 51 high mass star forming cores associated with water masers at 350 micron. The spectral energy distributions
We apply standard, first-principles calculations to a complete treatment of lattice dynamics in the harmonic approximation. The algorithm makes use
Our knowledge of the initial conditions and early stages of high mass star formation is very limited. We will review