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Is it feasible to perform space VLBI at 230 GHz? Also how does one detect the radio jets at 230 GHz?
The calculation of radio antenna gain at 230 GHz involves understanding the power radiated by the source, specifically bolometric luminosity, which is noted as 1036 erg/s in this discussion. The Event Horizon Telescope serves as a relevant example of a mm-VLBI instrument that operates effectively at this frequency, utilizing the CARMA array for observations. The discussion highlights the significance of 230 GHz as it corresponds to strong transition lines for carbon monoxide, making it crucial for detecting radio jets and mapping black hole jets. Additionally, the resolution of millimeter VLBI is well-suited for studying inner disk physics around black holes.
PREREQUISITESAstronomers, astrophysicists, and researchers involved in radio astronomy, particularly those focusing on high-frequency observations and black hole studies.