Direct Evidence of Two-component Ejecta in Supernova 2016gkg from Nebular Spectroscopy*
Jerkstrand A; Folatelli G; Kravtsov T; Lyman JD; Gutierrez CP; Bersten MC; Mattila S; Kuncarayakti H; Garcia F; Sanchez SF; Anderson JP; Ferrari L; Olivares EF; Maeda K; Kawabata KS; Galbany L; Van Dyk SD; Dessart L; Hattori T; Aoki K
Direct Evidence of Two-component Ejecta in Supernova 2016gkg from Nebular Spectroscopy*
Jerkstrand A
Folatelli G
Kravtsov T
Lyman JD
Gutierrez CP
Bersten MC
Mattila S
Kuncarayakti H
Garcia F
Sanchez SF
Anderson JP
Ferrari L
Olivares EF
Maeda K
Kawabata KS
Galbany L
Van Dyk SD
Dessart L
Hattori T
Aoki K
IOP PUBLISHING LTD
Julkaisun pysyvä osoite on:
https://urn.fi/URN:NBN:fi-fe2021042824862
https://urn.fi/URN:NBN:fi-fe2021042824862
Tiivistelmä
Spectral observations of the type-IIb supernova (SN) 2016gkg at 300-800 days are reported. The spectra show nebular characteristics, revealing emission from the progenitor star's metal-rich core and providing clues to the kinematics and physical conditions of the explosion. The nebular spectra are dominated by emission lines of [O i] lambda lambda 6300, 6364 and [Ca ii] lambda lambda 7292, 7324. Other notable, albeit weaker, emission lines include Mg I] lambda 4571, [Fe ii] lambda 7155, O I lambda 7774, Ca II triplet, and a broad, boxy feature at the location of H alpha. Unlike in other stripped-envelope SNe, the [O i] doublet is clearly resolved due to the presence of strong narrow components. The doublet shows an unprecedented emission line profile consisting of at least three components for each [O i]lambda 6300, 6364 line: a broad component (width similar to 2000 km s(-1)), and a pair of narrow blue and red components (width similar to 300 km s(-1)) mirrored against the rest velocity. The narrow component appears also in other lines, and is conspicuous in [O i]. This indicates the presence of multiple distinct kinematic components of material at low and high velocities. The low-velocity components are likely to be produced by a dense, slow-moving emitting region near the center, while the broad components are emitted over a larger volume. These observations suggest an asymmetric explosion, supporting the idea of two-component ejecta that influence the resulting late-time spectra and light curves. SN 2016gkg thus presents striking evidence for significant asymmetry in a standard-energy SN explosion. The presence of material at low velocity, which is not predicted in 1D simulations, emphasizes the importance of multidimensional explosion modeling of SNe.
Kokoelmat
- Rinnakkaistallenteet [19207]