Mini-supernovae from white dwarf–neutron star mergers: Viewing-angle-dependent spectra and light curves

Open Access

Fig. 3.

Emergent spectra of WD–NS mSNe for θ_view = 0°, 15°, 30°, 45°, 60°, and 90°. Colored lines show the total observed emergent spectra at different epochs following the WD–NS merger of our fiducial model, assuming a luminosity distance of D_L = 10 pc. The derived photospheric blackbody temperatures, $T_{phot}^{BB}$ $T^{\mathrm{BB}}_{\mathrm{phot}}$ , are indicated in the labels.

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