activity
20072021
most citedFirst proper motions of thin dust filaments at the Galactic Center

69 citations · 391 across the 10 of their papers we have counts for

collaborators

8 papers

astro-ph.SR2021★ 25 cited

Youth analysis of near infrared spectra of young low-mass stars and brown dwarfs

V. Almendros-Abad, K. Mužić, A. Moitinho +2

We aim at building a method that efficiently identifies young low-mass stars and brown dwarfs from low-resolution near-infrared spectra, by studying gravity-sensitive features and…

astro-ph.SR2014★ 23 cited

Properties of bow-shock sources at the Galactic center

J. Sanchez-Bermudez, R. Schödel, A. Alberdi +3

There are an enigmatic population of massive stars around the Galactic Center (GC) that were formed some Ma ago. A fraction of these stars has been found to orbit the supermassive…

astro-ph.GA2012★ 30 cited

The Galactic centre mini-spiral in the mm-regime

D. Kunneriath, A. Eckart, S. N. Vogel +10

The mini-spiral is a feature of the interstellar medium in the central ~2 pc of the Galactic center. It is composed of several streamers of dust and ionised and atomic gas with tem…

astro-ph.GA2010★ 32 cited

Coordinated NIR/mm observations of flare emission from Sagittarius A*

D. Kunneriath, G. Witzel, A. Eckart +28

We report on a successful, simultaneous observation and modelling of the millimeter (mm) to near-infrared (NIR) flare emission of the Sgr A* counterpart associated with the superma…

astro-ph.CO2009★ 52 cited

Modeling mm- to X-ray flare emission from SgrA*

A. Eckart, F. K. Baganoff, M. R. Morris +17

We report on new modeling results based on the mm- to X-ray emission of the SgrA* counterpart associated with the massive black hole at the Galactic Center. Our modeling is based o…

astro-ph2008★ 5 cited

Coordinated mm/sub-mm observations of Sagittarius A* in May 2007

D. Kunneriath, A. Eckart, S. Vogel +26

At the center of the Milky Way, with a distance of ~8 kpc, the compact source Sagittarius A* (SgrA*) can be associated with a super massive black hole of ~4x10^6 solar masses. SgrA…