Very Large Array Observations of Winds from Massive Stars

As mentioned before, although there has been no research using ML in the estimation of radio propagation loss in the presence of vegetation, there are some works related to

The detection of radio emission in Swift J0243.6+6124 (a high-mass neutron star binary) has also been interpreted as coming from a jet based on the correlation between X-ray and

As a first step, we verify the analysis procedure using simu- lated point-like sources with the computed spectra correspond- ing to (1) the inner part of the lunar disk (the total

A comparison between the radio and X-ray populations in Orion shows that the radio detections so far have been strongly biased to the brighter X-ray stars. This supports the

As a first step in our study, we characterized the mid-IR high-ionization emission lines produced by AGN and star-formation for a large sample of local galaxies, includ- ing

In this letter we present the results for three stars from the DUNES sam- ple (α Men, HD 88230, and HD 210277) as clear examples of the advantages offered by Herschel observations:

In a similar way we can determine the cumulative fraction of clusters that host diffuse relic emission as a function of radio flux. 7 shows the cumulative fraction for different

In conclusion, we have demonstrated that autophagic flux is impaired in livers from both patients and murine models of NAFLD, as well as in long-term PA-loaded human Figure 7 Efect