![Volker Heesen on Twitter: "What is now new is the clear connection with the radio spectral index. More massive galaxies (higher mass, SFR, size, rotation speed) have steeper radio spectra, so that Volker Heesen on Twitter: "What is now new is the clear connection with the radio spectral index. More massive galaxies (higher mass, SFR, size, rotation speed) have steeper radio spectra, so that](https://pbs.twimg.com/media/FPkXLjkXEAQCmNv.png)
Volker Heesen on Twitter: "What is now new is the clear connection with the radio spectral index. More massive galaxies (higher mass, SFR, size, rotation speed) have steeper radio spectra, so that
![Relationship between the X-ray luminosity and the SFR This figure shows... | Download Scientific Diagram Relationship between the X-ray luminosity and the SFR This figure shows... | Download Scientific Diagram](https://www.researchgate.net/publication/336540317/figure/fig3/AS:814132827803649@1571115800098/Relationship-between-the-X-ray-luminosity-and-the-SFR-This-figure-shows-the-scaling.png)
Relationship between the X-ray luminosity and the SFR This figure shows... | Download Scientific Diagram
![For each galaxy in our sample, we plot the 4.85 GHz radio luminosity of... | Download Scientific Diagram For each galaxy in our sample, we plot the 4.85 GHz radio luminosity of... | Download Scientific Diagram](https://www.researchgate.net/publication/51946449/figure/fig4/AS:347418081153024@1459842333300/For-each-galaxy-in-our-sample-we-plot-the-485GHz-radio-luminosity-of-its-brightest-SNR.png)