EMIG https://hdl.handle.net/1887/3160759

Combined constraints: gas temperature and density The constraints imposed on the gas properties by the inte- grated optical depth of the C280α and C351α lines and the ratio of

The detection of low-frequency RRLs is greatly aided to- wards bright radio sources as the intensity of stimulated tran- sitions is proportional to the strength of the radio

However, this value is based on a limited number of objects, and the method of computing the distance to a region using the measured distances to its confirmed members cannot be

Lenouvel F, Fraissinet-Tachet L, van de Vondervoort PJI, Visser J (2001) Isolation of UV-induced mutations in the areA nitrogen regulatory gene of Aspergillus niger, and construction

Our aim is to (i) determine if observations with LOFAR in this frequency range can yield CRRL detections, (ii) test if the integrated optical depth of the lines at high

While several calculations of RR rates, including total rates and /or detailed rate coefficients, for different isoelectronic se- quences are available, for example, Gu (2003)

For a different set of 14 ETGs (see Table A6), we detect emission in our lower resolution 1.4 GHz data, but not in the high-resolution 5 GHz data presented in Nyland et al. In

Combined model constraints for the CRRL integrated optical depth ( τ) and linewidth (FWHM) for the Perseus arm component at −47 km s −1.. The 1, 2 and 3 σ confidence limits from