Iptf13dcc
WebThe explosion mechanism of broad-lined type Ic supernovae (SNe Ic-BL) is not very well understood despite their discovery more than two decades ago. Recently a serious confrontation of SNe Ic-BL... http://export.arxiv.org/abs/1609.08145v1
Iptf13dcc
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WebJan 20, 2024 · We present the light curves of the hydrogen-poor superluminous supernovae (SLSNe-I) PTF12dam and iPTF13dcc, discovered by the (intermediate) Palomar … WebFeb 23, 2024 · In this paper, we investigate two hydrogen-poor superluminous supernovae (SLSNe) iPTF15esb and iPTF13dcc whose light curves (LCs) show significant deviation …
WebThe two fainter galaxies (iPTF13dcc with V~23.6 and iPTF13ehe with 21) still host the ongoing supernova (equal in brightness or fainter than the galaxy) and we will observe them with ACS with one filter (F625W). We intend to divide each orbit in a few sub-exposures and dither them to correct for cosmic rays and bad pixels. 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.
Webof PTF12dam and iPTF13dcc; Liu et al. (2024) develop a multiple CSI model involving the collisions between the ejecta and the CSM shells or winds locating at different sites and use these models to fit the LCs of iPTF15esb and iPTF13dcc. In this paper, we study two hydrogen-poor SNe, PS1-12cil and SN 2012aa. PS1-12cil is an SLSN I discovered ... WebGet DTF13-12PA DEUTSCH Automotive Headers specs, pricing, inventory availability, and more from TE Connectivity. Get a sample or request a quote.
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"
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... green waste of tehama landfillWebA Multiple Ejecta-circumstellar Medium Interaction Model and Its Implications for Superluminous Supernovae iPTF15esb and iPTF13dcc The Astrophysical Journal 2024-03-26 Journal article fn.gg most wantedWebThe hydrogen-poor superluminous supernova iPTF13ajg and its host galaxy in absorption and emission fn gg rebootallyWebSomehow this event is getting removed before the import completes. It appears that the data is being imported when its task is run (the ascii task), but it is not surviving cleanup. green waste of tehama jobsWebUsing 1D, non-local thermodynamic equilibrium and time-dependent radiative transfer simulations, we study the ejecta properties required to match the early- and late-time photometric and... fn gg realityWebFeb 20, 2024 · In this paper, we investigate two hydrogen-poor superluminous supernovae (SLSNe) iPTF15esb and iPTF13dcc whose light curves (LCs) show significant deviation … fn gg item shopWebSep 26, 2024 · The Intermediate Palomar Transient Factory reported the discovery of an unusual type II-P supernova iPTF14hls. Instead of an ∼100 day plateau as observed for ordinary type II-P supernovae, the light curve of iPTF14hls has at least five distinct peaks, followed by a steep decline at ∼1000 days since discovery. green waste of tehama ca