Toward an inner connection of SNe Ic, SLSNe Ic, XRF connected SNe, SNe Ic-BL, and GRB connected SNe
arXiv:1803.11402 · doi:10.1017/pasa.2018.35
Abstract
Type Ic supernovae (SNe) can be classified as: normal SNe Ic, type Ic super-luminous SNe (SLSNe Ic), X-ray flash (XRF) connected SNe, broad-line SNe Ic (SN Ic-BL), and gamma-ray burst (GRB) connected SNe. Here we suggest an inner connection for all kinds of SNe Ic based on a pair of jets being successfully launched: a normal SN Ic is a normal core collapsar without jets launched; a GRB associated SN Ic is a core collapsar with relativistic jets launched and successfully breaking out the envelope of the progenitor; an XRF associated SN Ic is a core collapsar with jets launched but can only develop a relativistic shock breakout; an SN Ic-BL is an off-axis GRB or XRF associated supernova; and an SLSN Ic is close to the XRF-SN Ic but the shock breakout is not relativistic and most of the jet energy is deposited into the supernova component. Based on the luminosity-distance diagram, we derived the luminosity function of all different types of SNe Ic as a whole. We also show that the normal SNe Ic and GRB connected SNe Ic have similar accumulative distributions.
References in corpus (32)
- The Supernova -- Gamma-Ray Burst Connection
- An optical supernova associated with the X-ray flash XRF 060218
- No supernovae associated with two long-duration gamma ray bursts
- An enigmatic long-lasting gamma-ray burst not accompanied by a bright supernova
- The metamorphosis of Supernova SN2008D/XRF080109: a link between Supernovae and GRBs/Hypernovae
- On the Rates of Gamma Ray Bursts and Type Ib/c Supernovae
- The Broad-lined Type Ic SN 2003jd
- Making a Short Gamma-Ray Burst from a Long one: Implications for the Nature of GRB 060614
- The Observable Signatures of GRB Cocoons
- The ultra-long Gamma-Ray Burst 111209A: the collapse of a blue supergiant?
- Long Gamma-Ray Bursts and Type Ic Core Collapse Supernovae Have Similar Locations in Hosts
- Hyper-accreting black hole as GRB central engine. I: Baryon loading in GRB jets
- A unified picture for low-luminosity and long gamma-ray bursts based on the extended progenitor of llgrb 060218/SN 2006aj
- Absolute-Magnitude Distributions of Supernovae
- The Connection between Gamma-Ray Bursts and Extremely Metal-Poor Stars: Black Hole-forming Supernovae with Relativistic Jets
- A Core-Collapse Supernova Model for the Extremely Luminous Type Ic Supernova 2007bi: An Alternative to the Pair-Instability Supernova Model
- Spectroscopic evidence for SN 2010ma associated with GRB 101219B
- An unexpectedly low-redshift excess of Swift gamma-ray burst rate
- A statistical study of super-luminous supernovae in the magnetar engine model and implications for their connection with gamma-ray bursts and hypernovae
- The GRB-SLSN Connection: mis-aligned magnetars, weak jet emergence, and observational signatures
- Shock Breakout in Type Ibc Supernovae and Application to GRB 060218/SN 2006aj
- A Common Central Engine for Long Gamma Ray Bursts and Type Ib/c Supernovae?
- A mildly relativistic radio jet from the otherwise normal Type Ic Supernova 2007gr
- The afterglow of a relativistic shock breakout and low-luminosity GRBs
- The supernova/gamma-ray burst/jet connection
- A Unified Energy-Reservoir Model Containing Contributions from Ni and Neutron Stars and Its Implication to Luminous Type Ic Supernovae
- Optical Follow-Up Observations of PTF10qts, a Luminous Broad-Lined Type Ic Supernova Found by the Palomar Transient Factory
- Relativistic Jets in Core Collapse Supernovae
- Collapsar Gamma-Ray Bursts: how the luminosity function dictates the duration distribution
- A new class of gamma-ray bursts from stellar disruptions by intermediate mass black holes
- Continuum spectral energy distribution of GRB, SLSN, SB and AGN host galaxies at intermediate redshifts
- A quick estimation of luminosity function based on the luminosity-distance diagram