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20012026
most citedAn Extremely Top-Heavy IMF in the Galactic Center Stellar Disks

383 citations · 1.2k across the 12 of their papers we have counts for

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6 papers · 1 filter

astro-ph2007★ 185 cited

The Initial Mass Function of the Massive Star-forming Region NGC 3603 from Near-Infrared Adaptive Optics observations

Y. Harayama, F. Eisenhauer, F. Martins

We study the initial mass function (IMF) of one of the most massive Galactic star-forming regions NGC 3603 to answer a fundamental question in current astrophysics: is the IMF univ…

astro-ph2007★ 128 cited

Evidence for a Long-Standing Top-Heavy IMF in the Central Parsec of the Galaxy

H. Maness, F. Martins, S. Trippe +10

We classify 329 late-type giants within 1 parsec of Sgr A*, using the adaptive optics integral field spectrometer SINFONI on the VLT. These observations represent the deepest spect…

astro-ph2006★ 75 cited

GCIRS16SW: a massive eclipsing binary in the Galactic Center

F. Martins, S. Trippe, T. Paumard +7

We report on the spectroscopic monitoring of GCIRS16SW, an Ofpe/WN9 star and LBV candidate in the central parsec of the Galaxy. SINFONI observations show strong daily spectroscopic…

astro-ph2006★ 61 cited

On the sensitivity of HeI singlet lines to the FeIV model atom in O stars

F. Najarro, D. J. Hillier, J. Puls +2

Recent calculations and analyses of O star spectra have revealed discrepancies between theory and observations, and between different theoretical calculations, for the strength of…

astro-ph2005★ 99 cited

Variations in the spectral slope of Sgr A* during a NIR flare

S. Gillessen, F. Eisenhauer, E. Quataert +10

We have observed a bright flare of Sgr A* in the near infrared with the adaptive optics assisted integral field spectrometer SINFON. Within the uncertainties, the observed spectrum…

astro-ph2001★ 162 cited

On the effective temperature scale of O stars

F. Martins, D. Schaerer, D. J. Hillier

We rediscuss the temperature of O dwarfs based on new non-LTE line blanketed atmosphere models including stellar winds computed with the CMFGEN code of Hillier & Miller (1998). Com…