We present new high-resolution observations of Sagittarius A* at wavelengths of 17.4-23.8 cm with the Very Large Array in the A configuration with the Pie Town Very Long Baseline Array (VLBA) antenna. We use the measured sizes to calibrate the interstellar scattering law and find that the major axis size of the scattering law is smaller by ~6% than previous estimates. Using the new scattering law, we are able to determine the intrinsic size of Sgr A* at wavelengths from 0.35 to 6 cm using existing results from the VLBA. The new law increases the intrinsic size by ~20% at 0.7 cm and <5% at 0.35 cm. The intrinsic size is 13<SUP>+7</SUP><SUB>-3</SUB>R<SUB>S</SUB> at 0.35 cm and is proportional to lambda<SUP>gamma</SUP>, where gamma is in the r...
Context. The compact radio source Sagittarius A∗ (Sgr A∗) in the Galactic centre is the primary supe...
At radio wavelengths, images of the compact radio source Sagittarius A* (Sgr A*) in the Galactic cen...
International audienceContext. The compact radio source Sagittarius A∗ (Sgr A∗) in the Galactic cent...
Contains fulltext : 35195.pdf ( ) (Open Access) ...
The radio emission from Sgr A* is thought to be powered by accretion onto a supermassive black hole ...
The radio emission from Sgr A* is thought to be powered by accretion onto a supermassive black hole ...
Recent proper motion studies of stars at the very center of the Galaxy strongly suggest that Sagitta...
We have detected the intrinsic size of Sagittarius A*, the Galac-tic Center radio source associated ...
We have detected the intrinsic size of Sagittarius A*, the Galactic center radio source associated w...
International audienceThe Galactic center supermassive black hole Sagittarius A* (Sgr A*) is one of ...
The Galactic center supermassive black hole Sagittarius A* (Sgr A*) is one of the most promising tar...
[[abstract]]Although it is widely accepted that most galaxies have supermassive black holes at their...
We present the highest resolution VLBI imaging observations of Sgr A* made at both 7 and 3.5 mm. The...
Recent radio observations by the Very Long Baseline Array at 7 and 3.5 mm produced the high-resoluti...
The Galactic center supermassive black hole Sagittarius A∗ (Sgr A∗) is one of the most promising tar...
Context. The compact radio source Sagittarius A∗ (Sgr A∗) in the Galactic centre is the primary supe...
At radio wavelengths, images of the compact radio source Sagittarius A* (Sgr A*) in the Galactic cen...
International audienceContext. The compact radio source Sagittarius A∗ (Sgr A∗) in the Galactic cent...
Contains fulltext : 35195.pdf ( ) (Open Access) ...
The radio emission from Sgr A* is thought to be powered by accretion onto a supermassive black hole ...
The radio emission from Sgr A* is thought to be powered by accretion onto a supermassive black hole ...
Recent proper motion studies of stars at the very center of the Galaxy strongly suggest that Sagitta...
We have detected the intrinsic size of Sagittarius A*, the Galac-tic Center radio source associated ...
We have detected the intrinsic size of Sagittarius A*, the Galactic center radio source associated w...
International audienceThe Galactic center supermassive black hole Sagittarius A* (Sgr A*) is one of ...
The Galactic center supermassive black hole Sagittarius A* (Sgr A*) is one of the most promising tar...
[[abstract]]Although it is widely accepted that most galaxies have supermassive black holes at their...
We present the highest resolution VLBI imaging observations of Sgr A* made at both 7 and 3.5 mm. The...
Recent radio observations by the Very Long Baseline Array at 7 and 3.5 mm produced the high-resoluti...
The Galactic center supermassive black hole Sagittarius A∗ (Sgr A∗) is one of the most promising tar...
Context. The compact radio source Sagittarius A∗ (Sgr A∗) in the Galactic centre is the primary supe...
At radio wavelengths, images of the compact radio source Sagittarius A* (Sgr A*) in the Galactic cen...
International audienceContext. The compact radio source Sagittarius A∗ (Sgr A∗) in the Galactic cent...