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20022020
most citedArray Programming with NumPy

23.6k citations

Showing astro-ph.GAShow all

8 papers · 1 filter

astro-ph.GA2019

Circumgalactic Gas and the Precipitation Limit

G. M. Voit, A. Babul, Iu. Babyk +15

During the last decade, numerous and varied observations, along with increasingly sophisticated numerical simulations, have awakened astronomers to the central role the circumgalac…

astro-ph.GA20193 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.GA20195 cited

Twelve Decades: Probing the Interstellar Medium from kiloparsec to sub-AU scales

Dan Stinebring, Shami Chatterjee, Susan E. Clark +15

After a decade of great progress in understanding gas flow into, out of, and through the Milky Way, we are poised to merge observations with simulations to build a comprehensive pi…

astro-ph.GA20199 cited

Envisioning the next decade of Galactic Center science: a laboratory for the study of the physics and astrophysics of supermassive black holes

Tuan Do, Andrea Ghez, Jessica R. Lu +38

As the closest example of a galactic nucleus, the Galactic center (GC) presents an exquisite laboratory for learning about supermassive black holes (SMBH) and their environment. We…

astro-ph.GA2019

Astro2020 Science White Paper: Science at the edges: internal kinematics of globular clusters' external fields

A. Bellini, M. Libralato, J. Anderson +17

The outer regions of globular clusters can enable us to answer many fundamental questions concerning issues ranging from the formation and evolution of clusters and their multiple…

astro-ph.GA2010

Testing stellar cusp formation theories with observations of the Milky Way nuclear star cluster

Tuan Do, Andrea M. Ghez, Mark R. Morris +5

(Abridged) We report on the structure of the nuclear star cluster in the innermost 0.16 pc of the Galaxy as measured by the number density profile of late-type giants. Using laser…