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20082026
most citedStellar Populations in the Central 0.5 pc of the Galaxy II: The Initial Mass Function

307 citations · 2.8k across the 70 of their papers we have counts for

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Showing 2019Show all

7 papers · 1 filter

astro-ph.GA2019★ 68 cited

A hidden friend for the galactic center black hole, Sgr A*

Smadar Naoz, Clifford M. Will, Enrico Ramirez-Ruiz +3

The hierarchical nature of galaxy formation suggests that a supermassive black hole binary could exist in our galactic center. We propose a new approach to constraining the possibl…

astro-ph.GA2019★ 18 cited

Consistency of the Infrared Variability of Sgr A* over 22 years

Zhuo Chen, E. Gallego-Cano, T. Do +14

We report new infrared measurements of the supermassive black hole at the Galactic Center, Sgr A*, over a decade that was previously inaccessible at these wavelengths. This enables…

astro-ph.IM2019★ 6 cited

High-resolution Infrared Spectrograph for Exoplanet Characterization with the Keck and Thirty Meter Telescopes

Dimitri Mawet, Michael Fitzgerald, Quinn Konopacky +46

HISPEC (High-resolution Infrared Spectrograph for Exoplanet Characterization) is a proposed diffraction-limited spectrograph for the W.M. Keck Observatory, and a pathfinder for the…

astro-ph.GA2019★ 97 cited

Unprecedented variability of Sgr A* in NIR

Tuan Do, Gunther Witzel, Abhimat K. Gautam +10

The electromagnetic counterpart to the Galactic center supermassive black hole, Sgr A*, has been observed in the near-infrared for over 20 years and is known to be highly variable.…

astro-ph.GA2019★ 3 cited

Astro2020 Science White Paper: The Local Relics of of Supermassive Black Hole Seeds

Jenny E Greene, Aaron Barth, Andrea Bellini +18

We have compelling evidence for stellar-mass black holes (BHs) of ~5-80 M_sun that form through the death of massive stars. We also have compelling evidence for so-called supermass…

astro-ph.GA2019★ 1 cited

Star Formation in Different Environments: The Initial Mass Function

M. W. Hosek, J. R. Lu, M. Andersen +7

The stellar initial mass function (IMF) is a fundamental property of star formation, offering key insight into the physics driving the process as well as informing our understandin…