We find that, for optically thick disks, CO inner radii are strongly correlated with the total system luminosity (stell... ▽ More We present an analysis of
CO emission lines from a sample of T Tauri, Herbig Ae / Be, and transitional disks with known inclinations, in order to study the structure of inner disk molecular gas.
Abstract: We present an analysis of
CO emission lines from a sample of T Tauri, Herbig Ae / Be, and transitional disks with known inclinations, in order to study the structure of inner disk molecular gas.
Not exact matches
To study the structure and kinematics of gas around IRAS 16547 - 4247, the research group observed molecular
line emission of dust,
CO, and methanol (CH3OH).
Recently, signatures of
CO Cameron and
CO2 + doublet ultraviolet auroral
emissions have been detected with SPICAM (Gérard et al. 2015); they showed that the Mars aurora is a temporary and spatially localized phenomenon appearing near the open - closed magnetic field
line boundary in cusp - like structures.
In order to cut
emissions quickly and effectively a collection of rare metal catalysts were embedded in a ceramic honeycomb structure to burn off the unburnt hydrocarbons and complete the conversion of
CO to
CO2 along with the NOx Clutch: A mechanism to disengage and apply power from the engine to the gearbox and drive
line.