Iptf13dcc
WebFig. 3.— Same as in Figure 1 but for iPTF13dcc. Data are obtained from Vreeswijk et al. (2024). The fitting parameters are shown in the text and Table 1. - "A Multiple Ejecta-Circumstellar Medium Interaction Model and Its Implications for Superluminous Supernovae iPTF15esb and iPTF13dcc" WebIn this paper, we investigate two hydrogen-poor superluminous supernovae (SLSNe), iPTF15esb and iPTF13dcc, whose light curves (LCs) show significant deviation from the …
Iptf13dcc
Did you know?
WebIn contrast, the long-duration (>30days) early excess emission in iPTF13dcc, whose brightness competes with that of the main peak, appears to be of a different nature. We construct bolometric light curves for both targets, and fit a variety of light-curve models to both the early bump and main peak in an attempt to understand the nature of WebA Multiple Ejecta-circumstellar Medium Interaction Model and Its Implications for Superluminous Supernovae iPTF15esb and iPTF13dcc The Astrophysical Journal 2024-03-26 Journal article
WebFeb 20, 2024 · In this paper, we investigate two hydrogen-poor superluminous supernovae (SLSNe) iPTF15esb and iPTF13dcc whose light curves (LCs) show significant deviation … WebWe present the light curves of the hydrogen-poor superluminous supernovae (SLSNe-I) PTF12dam and iPTF13dcc, discovered by the (intermediate) Palomar Transient...
WebWell sampled light curves of SN2015bn and iPTF13dcc have also resulted in discov- eries of LC undulations of SLSNe-I, suggesting possible ejecta interaction with H-poor CSM (Nicholl et al. 2016; Vreeswijk et al. 2024). In this paper, we report two new SLSNe-I events, iPTF15esb and iPTF16bad, showing late-time H emis- sion, similar to iPTF13ehe. WebSep 26, 2016 · A model combining a shock breakout in an extended envelope with late-time magnetar energy injection provides a reasonable fit to the iPTF13dcc observations. …
WebThe spectra of iPTF16asu and iPTF13dcc (fig. 5 in Vreeswijk et al. 2024) near peak are pretty featureless, consistent with CSM–ejecta SNe. However, the spectra of iPTF15esb (fig. 1 in Yan et al. 2024) near peak light show prominent absorption at rest frame ∼ 4100 ˚A.
WebJan 20, 2024 · We present the light curves of the hydrogen-poor superluminous supernovae (SLSNe-I) PTF12dam and iPTF13dcc, discovered by the (intermediate) Palomar Transien... shure m1 cartridgehttp://export.arxiv.org/abs/1609.08145v1 the outwaters metacriticWebIn this paper, we investigate two hydrogen-poor superluminous supernovae (SLSNe), iPTF15esb and iPTF13dcc, whose light curves (LCs) show significant deviation from the … the outwaters free onlineWebIn this paper, we investigate two hydrogen-poor superluminous supernovae (SLSNe) iPTF15esb and iPTF13dcc whose light curves (LCs) show significant deviation from the smooth rise and fall. The LC of iPTF15esb exhibits two peaks and a post-peak plateau, and furthermore the late-time spectrum of iPTF15esb shows a strong, broad H α emission … the outwaters filme completoWebSep 27, 2016 · We present the light curves of the hydrogen-poor superluminous supernovae (SLSNe-I) PTF12dam and iPTF13dcc, discovered by the (intermediate) Palomar Transient Factory. Both show excess emission at … shure m21 cartridgeWebJan 20, 2024 · We present the light curves of the hydrogen-poor superluminous supernovae (SLSNe-I) PTF12dam and iPTF13dcc, discovered by the (intermediate) Palomar … shure lyric monitorWebMar 26, 2024 · This site uses cookies. By continuing to use this site you agree to our use of cookies. To find out more, see our the outwaters film wiki