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The First Hours and Days of the 2021 Explosion of the Recurrent Symbiotic Nova RS Ophiuchii

  • Authors: Augustin Skopal, Martin Vrašťák, Francois Teyssier, Mitsugu Fujii, Sergei Shugarov, Miroslav Šlechta, Marek Wolf

Augustin Skopal et al 2026 The Astrophysical Journal 1007 .

  • Provider: AAS Journals

Caption: Figure 8.

Evolution of the Hα line parameters. Left: the broad component is shown. The flux (panel (a)), its maximum height, ﹩{F}_{{\rm{\max }}}﹩, above the continuum (panel (b)), FWHM (panel (c)), and terminal velocities of the wings (panel (d)) are detailed. A description of these panels is in Section 3.5.1, and the data are given in Table 9. Right: the narrow components are shown. The fluxes (panel (e)), FWZI of the absorption (panel (f)) and emission (panel (g)) component, and their radial velocities (panel (h)) are depicted. Their description and interpretation can be found in Sections 3.5.2 and 4.5, respectively.

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