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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Positions of radio galaxies, clusters, and 2-micron luminous galaxies correlate with the Local Supercluster plane at 100-200 Mpc, with tentative evidence at 400 Mpc.
Homogeneous [Fe/H] measurements for 334 Local Volume galaxies reveal a luminosity-metallicity relation [Fe/H] = -2.6 - 0.075 M_B with a distribution peaking at -1.89 dex.
42 supernova remnants confirmed in NGC3344 via [S II]/Hα selection, Sabbadin plots, BPT diagrams and shock models from SITELLE data.
citing papers explorer
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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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The Extended Plane of the Local Supercluster
Positions of radio galaxies, clusters, and 2-micron luminous galaxies correlate with the Local Supercluster plane at 100-200 Mpc, with tentative evidence at 400 Mpc.
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The Metal Content of Resolved Galaxies
Homogeneous [Fe/H] measurements for 334 Local Volume galaxies reveal a luminosity-metallicity relation [Fe/H] = -2.6 - 0.075 M_B with a distribution peaking at -1.89 dex.
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3D Optical Spectroscopic Study of NGC3344 with SITELLE: I. Identification and Confirmation of Supernova Remnants
42 supernova remnants confirmed in NGC3344 via [S II]/Hα selection, Sabbadin plots, BPT diagrams and shock models from SITELLE data.