Abstract.
We have developed a time-dependent model of ionization, excitation and energy balance of the atmosphere of SN 1987A at the photospheric epoch to study early behavior of hydrogen and helium lines. The ionization freeze-out effects play a key role in producing both the strong H\(\alpha\) during nearly the first month and the He I 5876 Å scattering line on day 1.76. Using an extended reaction network between hydrogen molecules and their ions demonstrates that ion-molecular processes are likely responsible for the blue peak in the H\({\alpha}\) profile at the Bochum event epoch.
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Utrobin, V.P., Chugai, N.N. Freeze-Out Effects in Hydrogen and Helium Lines of SN 1987A at the Early Photospheric Epoch. In: Hillebrandt, W., Leibundgut, B. (eds) From Twilight to Highlight: The Physics of Supernovae. ESO ASTROPHYSICS SYMPOSIA. Springer, Berlin, Heidelberg. https://doi.org/10.1007/10828549_34
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DOI: https://doi.org/10.1007/10828549_34
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Publisher Name: Springer, Berlin, Heidelberg
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