We report on new developments in VLBI, with emphasis on experiments performed at the highest frequencies possible to date (so called mm-VLBI). We have observed the nucleus of M 87 (Virgo A) with global VLBI at 3 mm. We show a new image of the inner-most jet region with an angular resolution of approx. 300 x 60 micro-arcseconds. In terms of Schwarzschild radii, this leads to an upper limit of the jet base of approx. 100 x 20 Schwarzschild radii. We also report on two VLBI pilot-experiments, which demonstrate the technical feasibility of global VLBI at 150 and 230 GHz (2 mm and 1.3 mm). The experiments lead to upper limits to the size of the unresolved AGN-cores in the 25 - 30 micro-arcsecond range. The participation of new and near-future mm...
Sagittarius A*, the ~4 × 106 M ☉ black hole candidate at the Galactic center, can be studied on Schw...
Very-long-baseline interferometry (VLBI) observations of active galactic nuclei at millimetre wavele...
Due to its proximity, M87 is a prime target for next-generation high-resolution VLBI at short millim...
Global VLBI imaging at millimeter and sub-millimeter wavelength overcomes the opacity barrier of syn...
Compact galactic and extragalactic radio sources can be imaged with an unsurpassed angular resolutio...
We summarize the present status of VLBI experiments at 3 mm (86 GHz), 2 mm (129-150 GHz) and 1.3 mm ...
We present and discuss new result from mm-VLBI observations of M87 and SgrA*, using the Global mm-VL...
At 147 GHz (2mm wavelength), we detected three prominent AGN (NRAO150, 3C279, 1633+382) with Very Lo...
Active galactic nuclei (AGN) are believed to be powered by accretion of gas onto a central supermass...
High-frequency VLBI is demonstrating its power with recent achievements such as imaging the shadow o...
Compact radio sources (Kellermann & Pauliny-Toth 1981) are widely accepted to be associated with sup...
We present 15 images from the global mm-VLBI sessions in 1990 April at 100GHz and 1993 April at 86GH...
We present 15 images from the global mm-VLBI sessions in 1990 April at 100GHz and 1993 April at 86GH...
The super-massive black holes (SMBH) located at the centres of AGN often launch highly relativistic ...
VLBA and Global VLBI observations of M87 at 43 GHz, some new and some previously published, are used...
Sagittarius A*, the ~4 × 106 M ☉ black hole candidate at the Galactic center, can be studied on Schw...
Very-long-baseline interferometry (VLBI) observations of active galactic nuclei at millimetre wavele...
Due to its proximity, M87 is a prime target for next-generation high-resolution VLBI at short millim...
Global VLBI imaging at millimeter and sub-millimeter wavelength overcomes the opacity barrier of syn...
Compact galactic and extragalactic radio sources can be imaged with an unsurpassed angular resolutio...
We summarize the present status of VLBI experiments at 3 mm (86 GHz), 2 mm (129-150 GHz) and 1.3 mm ...
We present and discuss new result from mm-VLBI observations of M87 and SgrA*, using the Global mm-VL...
At 147 GHz (2mm wavelength), we detected three prominent AGN (NRAO150, 3C279, 1633+382) with Very Lo...
Active galactic nuclei (AGN) are believed to be powered by accretion of gas onto a central supermass...
High-frequency VLBI is demonstrating its power with recent achievements such as imaging the shadow o...
Compact radio sources (Kellermann & Pauliny-Toth 1981) are widely accepted to be associated with sup...
We present 15 images from the global mm-VLBI sessions in 1990 April at 100GHz and 1993 April at 86GH...
We present 15 images from the global mm-VLBI sessions in 1990 April at 100GHz and 1993 April at 86GH...
The super-massive black holes (SMBH) located at the centres of AGN often launch highly relativistic ...
VLBA and Global VLBI observations of M87 at 43 GHz, some new and some previously published, are used...
Sagittarius A*, the ~4 × 106 M ☉ black hole candidate at the Galactic center, can be studied on Schw...
Very-long-baseline interferometry (VLBI) observations of active galactic nuclei at millimetre wavele...
Due to its proximity, M87 is a prime target for next-generation high-resolution VLBI at short millim...