activity
20062008
most citedPolarized NIR and X-ray Flares from SgrA*

93 citations · 260 across the 6 of their papers we have counts for

collaborators

6 papers

astro-ph200866 cited

A 600 minute near-infrared lightcurve of Sagittarius A*

L. Meyer, T. Do, A. Ghez +5

We present the longest, by a factor of two, near-infrared lightcurve from Sgr A* - the supermassive black hole in the Galactic center. Achieved by combining Keck and VLT data from…

astro-ph200843 cited

IRS 13N: a new comoving group of sources at the Galactic Center

K. Muzic, R. Schoedel, A. Eckart +2

Context: The Galactic Center IRS 13E cluster is located ~3.2'' from SgrA*. It is an extremely dense stellar association containing several Wolf-Rayet and O-type stars, at least fou…

astro-ph200793 cited

Polarized NIR and X-ray Flares from SgrA*

A. Eckart, F. K. Baganoff, M. Zamaninasab +18

Stellar dynamics indicate the presence of a super massive 3-4x10^6 Msun solm black hole at the Galactic Center. It is associated with the variable radio, near-infrared, and X-ray c…

astro-ph20071 cited

Flares from spiral waves by lensing and time-delay amplification?

V. Karas, M. Dovciak, A. Eckart +1

Episodically accreting black holes are thought to produce flares when a chunk of particles is accelerated to high velocity near the black hole horizon. This also seems to be the ca…

astro-ph200757 cited

On the orientation of the Sagittarius A* system

L. Meyer, R. Schoedel, A. Eckart +3

The near-infrared emission from the black hole at the Galactic center (Sgr A*) has unique properties. The most striking feature is a suggestive periodic sub-structure that has been…

astro-ph2006

The possibility of detecting Sagittarius A* at 8.6 mum

R. Schoedel, A. Eckart, K. Muzic +3

The Galactic Center was observed at 8.6 mum in order to detect a mid-infrared (MIR) counterpart of Sgr A*, parallel to NIR observations. The goal was to set constraints on possible…