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20242026
most citedGone with the Wind: JWST-MIRI Unveils a Strong Outflow from the Quiescent Stellar-Mass Black Hole A0620-00

1 citations · 2 across the 12 of their papers we have counts for

collaborators

14 papers

astro-ph.HE2026

JWST/MIRI Spectroscopy of the Quiescent Black Hole X-ray Binary XTE J1118+480: Constraints on Jet and Circumbinary Dust Contributions to the Mid-infrared Emission

Zihao Zuo, Elena Gallo, Nuria Calvet +9

We report on JWST/MIRI low-resolution spectroscopy (-m) and imaging (-m) of the black hole X-ray binary XTE~J1118+480 in quiescence, at an X-ray luminosity nine…

astro-ph.HE2026

The Demographics of Sagittarius A* X-ray Flares over 25 Years with Chandra

Zach Sumners, Nicole M. Ford, Daryl Haggard +10

We present the Chandra 25-year Sagittarius A* (Sgr A*) X-ray flare catalog: a systematic analysis of 6.8 Ms of Sgr A* monitoring spanning the Chandra X-ray Observatory's mission li…

astro-ph.GA2026

Ionization Structure and Metal Enrichment of the Galactic Center Minispiral Observed with JWST

Nicole M Ford, Mayura Balakrishnan, Sebastiano D. von Fellenberg +11

Sagittarius A* (Sgr A*) is the nearest quiescent supermassive black hole, and its proximity offers a unique opportunity to study its surrounding fuel supply. We leverage extensive…

astro-ph.HE2026

Infrared Line Diagnostics Fail to Constrain Sgr A*'s UV Output

Mayura Balakrishnan, Sebastiano D. von Fellenberg, Daryl Haggard +11

Sgr A*, the 4 x supermassive black hole at the Galactic Center, exhibits frequent flaring with X-ray luminosities of erg s, while i…

astro-ph.HE2026

Detection and Evolution of Linear Polarization of the Galactic Center Transient MAXI J1744-294

Joseph M. Michail, Sebastiano D. von Fellenberg, Mayura Balakrishnan +14

MAXI J1744294, likely a low-mass X-ray binary system, is a Galactic-center transient source, detected at radio and X-ray wavelengths, located approximately southeast of S…

astro-ph.HE2026

A Therapy Session with Sgr A*

Mayura Balakrishnan, Robert Frazier, Joseph Michail

The nature of Sagittarius A* (Sgr A*) has been the subject of intense study and debate for over half a century. Herein, we present the first successful interview with an astrophysi…

astro-ph.HE2025

Simultaneous JWST, NuSTAR, and VLA Monitoring of Sgr A*: A Unified Picture of the Variable IR, X-ray and Radio Emission

F. Yusef-Zadeh, M. Wardle, R. G. Arendt +5

Flux variability is a fundamental channel of information from Sgr A* because of its direct probe of processes occurring within an accretion disk under strong gravity. We present si…

astro-ph.GA2025★ 1 cited

Photometric Constraints on Intermediate-mass Black Holes in the Galactic Centre

Tamojeet Roychowdhury, Sebastiano D. von Fellenberg, Joseph M. Michail +14

JWST/MIRI observations can place photometric limits on the presence of an intermediate-mass black hole (IMBH) near the Galactic Centre. The stellar complex IRS 13E, a co-moving con…

astro-ph.HE2025

First Mid-infrared Detection and Modeling of a Flare from Sgr A*. II. Mid-IR Spectral Energy Distribution and Millimeter Polarimetry

Joseph M. Michail, Sebastiano D. von Fellenberg, Garrett K. Keating +20

S. D. von Fellenberg et al. (2025a, Paper I) reported the first mid-infrared detection of a flare from Sgr A*. The JWST/MIRI/MRS observations were consistent with an orbiting hotsp…

astro-ph.GA2025

Parsec-scale SiO emission in the Galactic Center

N. Wenner, C. J. Chandler, J. M. Michail +2

The central 5 parsecs of our Galactic Center is rich in various molecular tracers. The region is observed to be hot, highly ionized, and volatile, resulting in complex chemistry an…

astro-ph.HE2025★ 1 cited

Gone with the Wind: JWST-MIRI Unveils a Strong Outflow from the Quiescent Stellar-Mass Black Hole A0620-00

Zihao Zuo, Gabriele Cugno, Joseph Michail +15

We present new observations of the black hole X-ray binary A0620-00 using the Mid-Infrared Instrument on the James Webb Space Telescope, during a state where the X-ray luminosity i…

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

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.HE2024

G359.13142-0.20005: A steep spectrum radio pulsar candidate with an X-ray counterpart running into the Galactic Center Snake (G359.1-0.2)

F. Yusef-Zadeh, Jun-Hui Zhao, R. Arendt +5

The Snake is a remarkable Galactic center radio filament with a morphology characterized by two kinks along its extent. The major and minor kinks are located where the f…