We quantified the effects of stellar feedback in RCW 49 by determining physical conditions different regions using [CII] 158 $\mu$m and [OI] 63 observations from SOFIA, $^{12}$CO (3-2) APEX H$_2$ line Spitzer telescopes. Large maps were observed with SOFIA telescopes, while only available towards three small areas. From our qualitative analysis, we found that 0-0 S(2) emission probes denser gas...

Abstract The emission mechanism for hard γ -ray spectra from supernova remnants (SNRs) is still a matter of debate. Recent multiwavelength observations the TeV source HESS J1912+101 show that it associated with an SNR age ∼100 kyr, making unlikely produce via leptonic processes. We analyzed Fermi and found extended spectrum. may represent peculiar stage evolution dominates acceleration cosmic r...

Forest inventory data were used to develop a standage-driven, stochastic predictor of unit-area, frequencyweighted lists of breast high tree diameters (DBH). The average of mean statistics from 40 simulation prediction sets of an independent 78-plot validation dataset differed from the observed validation means by 0.5 cm for DBH, and by 12 trees/h for density. The 40simulation average of standa...