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Accretion-driven Sources in Spatially Resolved Lyα Emitters

  • Authors: Benjamin Dittenber, M. S. Oey, Edmund Hodges-Kluck, Elena Gallo, Matthew Hayes, Göran Östlin, and Jens Melinder

2020 The Astrophysical Journal Letters 890 L12.

  • Provider: AAS Journals

Caption: Figure 3.

LX–SFR–metallicity relation for star-forming galaxies, showing our sample and the relation from Brorby et al. (2016; blue line). Their observed 0.34 dex dispersion in the relation is shown by the gray band. Hardness ratio is indicated with the shown color scale; red points indicate objects without enough counts for a reliable HR estimate. Circles show Chandra ACIS observations, with point size scaled to source FWHM; diamonds indicate XMM data, which cannot resolve point sources in our sample. Haro 11-B is not a significant LAE, but is included for completeness. Data for Haro 11 and NGC 6090 are shown for individual subregions, as well as for total integrated values.

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