activity
20082023
most citedAn Extremely Top-Heavy IMF in the Galactic Center Stellar Disks

383 citations · 871 across the 6 of their papers we have counts for

collaborators

6 papers

astro-ph.IM2023★ 3 cited

The ESO Science Archive Facility: Status, Impact, and Prospects

Martino Romaniello, Magda Arnaboldi, Mauro Barbieri +14

Scientific data collected at ESO's observatories are freely and openly accessible online through the ESO Science Archive Facility. In addition to the raw data straight out of the i…

astro-ph.GA2023★ 11 cited

VISIONS: The VISTA Star Formation Atlas -- I. Survey overview

Stefan Meingast, João Alves, Hervé Bouy +37

VISIONS is an ESO public survey of five nearby (d < 500 pc) star-forming molecular cloud complexes that are canonically associated with the constellations of Chamaeleon, Corona Aus…

astro-ph.GA2010

Massive Young Stars in the Galactic Center

H. Bartko

We summarize our latest observations of the nuclear star cluster in the central parsec of the Galaxy with the adaptive optics assisted, integral field spectrograph SINFONI on the E…

astro-ph.GA2009★ 383 cited

An Extremely Top-Heavy IMF in the Galactic Center Stellar Disks

H. Bartko, F. Martins, S. Trippe +19

We present new observations of the nuclear star cluster in the central parsec of the Galaxy with the adaptive optics assisted, integral field spectrograph SINFONI on the ESO/VLT. O…

astro-ph.GA2009★ 193 cited

Evidence for X-ray synchrotron emission from simultaneous mid-IR to X-ray observations of a strong Sgr A* flare

K. Dodds-Eden, D. Porquet, G. Trap +22

This paper reports measurements of Sgr A* made with NACO in L' -band (3.80 um), Ks-band (2.12 um) and H-band (1.66 um) and with VISIR in N-band (11.88 um) at the ESO VLT, as well a…

astro-ph2008★ 281 cited

Evidence for Warped Disks of Young Stars in the Galactic Center

H. Bartko, F. Martins, T. K. Fritz +18

The central parsec around the super-massive black hole in the Galactic Center hosts more than 100 young and massive stars. Outside the central cusp (R~1") the majority of these O a…