{ "id": "2404.03112", "version": "v1", "published": "2024-04-03T23:25:18.000Z", "updated": "2024-04-03T23:25:18.000Z", "title": "On the Formation of the W-shaped O II Lines in Spectra of Type I Superluminous Supernovae", "authors": [ "Sei Saito", "Masaomi Tanaka", "Paolo A. Mazzali", "Stephan Hachinger", "Kenta Hotokezaka" ], "comment": "19 pages, 11 figures, accepted for publication in ApJ", "categories": [ "astro-ph.HE", "astro-ph.SR" ], "abstract": "H-poor superluminous supernovae (SLSNe-I) are characterized by O II lines around 4,000 - 4,500 A in pre-/near-maximum spectra, so-called W-shaped O II lines. As these lines are from relatively high excitation levels, they have been considered a sign of non-thermal processes, which may give a hint of power sources of SLSNe-I. However, the conditions for these lines to appear have not been understood well. In this work, we systematically calculate synthetic spectra to reproduce observed spectra of eight SLSNe-I, parameterizing departure coefficients from the nebular approximation in the SN ejecta (expressed as b_neb). We find that most of the observed spectra can be reproduced well with b_neb ~< 10, which means that no strong departure is necessary for the formation of the W-shaped O II lines. We also show that the appearance of the W-shaped O II lines is sensitive to temperature; only spectra with temperatures T ~ 14,000 - 16,000 K can produce the W-shaped O II lines without large departures. Based on this, we constrain the non-thermal ionization rate near the photosphere. Our results suggest that spectral features of SLSNe-I can give independent constraints on the power source through the non-thermal ionization rates.", "revisions": [ { "version": "v1", "updated": "2024-04-03T23:25:18.000Z" } ], "analyses": { "keywords": [ "superluminous supernovae", "non-thermal ionization rate", "power source", "relatively high excitation levels", "independent constraints" ], "note": { "typesetting": "TeX", "pages": 19, "language": "en", "license": "arXiv", "status": "editable" } } }