First polarization measurements of MAXI J1744-294 reveal a common Faraday screen with RM = -63606 rad m^{-2} matching the Galactic center magnetar, confirming the transient's location in the nuclear star cluster and suggesting an intrinsic RM for Sgr A*.
A., Tsutsumi, T., Brogan, C
3 Pith papers cite this work. Polarity classification is still indexing.
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2026 3representative citing papers
JWST, Subaru, and ALMA observations of HH 270 identify a new collimated jet closer to the source and show interactions between the shock-excited jet and the molecular outflow.
Multi-phase molecular gas in IRAS20551-4250 is dominated by cold CO, shows UV-heated warm H2, tidal features from a merger, and no molecular outflows, consistent with ongoing star formation.
citing papers explorer
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Detection and Evolution of Linear Polarization of the Galactic Center Transient MAXI J1744-294
First polarization measurements of MAXI J1744-294 reveal a common Faraday screen with RM = -63606 rad m^{-2} matching the Galactic center magnetar, confirming the transient's location in the nuclear star cluster and suggesting an intrinsic RM for Sgr A*.
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A Study of HH 270 with the James Webb Space Telescope
JWST, Subaru, and ALMA observations of HH 270 identify a new collimated jet closer to the source and show interactions between the shock-excited jet and the molecular outflow.
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GOALS-JWST: Resolved multi-phase molecular gas in IRAS 20551-4250 using JWST and ALMA
Multi-phase molecular gas in IRAS20551-4250 is dominated by cold CO, shows UV-heated warm H2, tidal features from a merger, and no molecular outflows, consistent with ongoing star formation.