HIGHLIGHTS
- who: Vollmer B. and collaborators from the Universitu00e9 Strasbourg, CNRS, Observatoire astronomique Strasbourg, UMR, Strasbourg, France Department, School Science, The Graduate University for Advanced Studies, SOKENDAI, Mitaka have published the paper: From the Circumnuclear Disk in the Galactic Center to thick, obscuring tori of AGNs - Modeling the molecular emission of a parsec-scale torus as found in NGC, in the Journal: (JOURNAL)
- what: The authors compare the resulting model datacubes the CO HCN HCO+ and CS brightness temperatures to available observations. Within the model, the disk is characterized by the disk mass accretion rate Mu0307 . . .
If you want to have access to all the content you need to log in!
Thanks :)
If you don't have an account, you can create one here.