Multi-phase observations of NGC 1427A indicate tidal torquing from a dwarf fly-by has pre-conditioned its gas for ram-pressure stripping by the Fornax intracluster medium, placing the galaxy at the onset of environmental quenching with a declining star formation rate.
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SIMLA delivers a complete set of cleaned mid-infrared spectral cubes (5.2-38 micron) from Spitzer/IRS mapping data for several hundred objects, processed via a novel pipeline and soon available at IRSA.
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Tidal pre-conditioning and ram-pressure stripping in NGC 1427A. Deep VLT/MUSE spectroscopy and FUV-to-radio observations trace a Fornax Cluster dwarf in transformation
Multi-phase observations of NGC 1427A indicate tidal torquing from a dwarf fly-by has pre-conditioned its gas for ram-pressure stripping by the Fornax intracluster medium, placing the galaxy at the onset of environmental quenching with a declining star formation rate.
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SIMLA: The Spitzer Infrared Spectrograph Mapping Legacy Archive
SIMLA delivers a complete set of cleaned mid-infrared spectral cubes (5.2-38 micron) from Spitzer/IRS mapping data for several hundred objects, processed via a novel pipeline and soon available at IRSA.