activity
20102026
most citedMassive Star Formation of the Sgr A East HII Regions Near the Galactic Center

30 citations · 30 across the 9 of their papers we have counts for

collaborators
Showing astro-ph.GAShow all

6 papers · 1 filter

astro-ph.GA2026

Observational Tests of Sgr A*'s State of the Accretion Flow

F. Yusef-Zadeh, R. G. Arendt, H. Bushouse +4

General relativistic magneto-hydrodynamic (GRMHD) simulations of the possibly magnetically arrested disk (MAD) of the accretion flow of Sgr A* predict short and long time variabili…

astro-ph.GA2025

A Catalog of Filaments in the Central Molecular Zone

Richard G. Arendt, F. Yusef-Zadeh, I. Heywood

We present a catalog of 1.28 GHz radio filaments observed by MeerKAT over the innermost 200 pc of the Galaxy (roughly ), which includes the central molecular zone (CMZ).…

astro-ph.GA2025

Non-stop Variability of Sgr A* using JWST at 2.1 and 4.8 micron Wavelengths: Evidence for Distinct Populations of Faint and Bright Variable Emission

F. Yusef-Zadeh, H. Bushouse, R. G. Arendt +3

We present first results of JWST Cycle 1 and 2 observations of Sgr A* using NIRCam taken simultaneously at 2.1 and 4.8 micron for a total of ~48 hours over seven different epochs i…

astro-ph.GA2024

Shockingly Bright Warm Carbon Monoxide Molecular Features in the Supernova Remnant Cassiopeia A Revealed by JWST

J. Rho, S. -H. Park, R. Arendt +36

We present JWST NIRCam (F356W and F444W filters) and MIRI (F770W) images and NIRSpec- IFU spectroscopy of the young supernova remnant Cassiopeia A (Cas A). We obtained the data as…

astro-ph.GA2024

The interaction of a large-scale nuclear wind with the high velocity HII region G0.17+0.15

F. Yusef-Zadeh, Jun-Hui Zhao, R. Arendt +4

We investigate the nature of a Galactic center source, G0.17+0.15, lying along the northern extension of the Radio Arc near l~0.2deg. G0.17+0.15 is an HII region located toward the…

astro-ph.GA2010★ 30 cited

Massive Star Formation of the Sgr A East HII Regions Near the Galactic Center

F. Yusef-Zadeh, J. H. Lacy, M. Wardle +4

A group of four compact HII regions associated with the well-known 50 km/s molecular cloud is the closest site of on-going star formation to the dynamical center of the Galaxy, at…