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- Publisher Website: 10.1017/pasa.2018.35
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Article: Toward an inner connection of SNe Ic, SLSNe Ic, XRF connected SNe, SNe Ic-BL, and GRB connected SNe
Title | Toward an inner connection of SNe Ic, SLSNe Ic, XRF connected SNe, SNe Ic-BL, and GRB connected SNe |
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Authors | |
Keywords | Gamma-ray bursts Stars: evolution Stars: jets Stars: massive Supernovae |
Issue Date | 2018 |
Publisher | Cambridge University Press. The Journal's web site is located at http://journals.cambridge.org/action/displayJournal?jid=pas |
Citation | Publications of the Astronomical Society of Australia, 2018, v. 35, article no. e032, p. 1-8 How to Cite? |
Abstract | Type Ic supernovae can be classified as normal supernovae Ic, type Ic super-luminous supernovae, X-ray flash-connected supernovae, broad-line supernovae Ic, and gamma-ray burst-connected supernovae. Here we suggest an inner connection for all kinds of supernovae Ic which is based on whether a pair of jets are successfully launched: a normal supernovae Ic is a normal core collapsar without jets launched; a gamma-ray burst-associated supernovae Ic is a core collapsar with relativistic jets launched and successfully breaking out the envelope of the progenitor; an X-ray flash-associated supernovae Ic is a core collapsar with jets launched but can only develop a relativistic shock breakout; a broad-line supernovae Ic is an off-axis gamma-ray burst or an X-ray flash-associated supernova; and a type Ic super-luminous supernovae is close to the X-ray flash-connected supernovae 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 supernovae Ic as a whole. We also show that the normal supernovae Ic and gamma-ray burst-connected supernovae Ic have similar accumulative distributions. |
Persistent Identifier | http://hdl.handle.net/10722/266044 |
ISSN | 2023 Impact Factor: 4.5 2023 SCImago Journal Rankings: 1.688 |
ISI Accession Number ID |
DC Field | Value | Language |
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dc.contributor.author | Zou, Y | - |
dc.contributor.author | Cheng, KS | - |
dc.date.accessioned | 2018-12-17T02:16:37Z | - |
dc.date.available | 2018-12-17T02:16:37Z | - |
dc.date.issued | 2018 | - |
dc.identifier.citation | Publications of the Astronomical Society of Australia, 2018, v. 35, article no. e032, p. 1-8 | - |
dc.identifier.issn | 1323-3580 | - |
dc.identifier.uri | http://hdl.handle.net/10722/266044 | - |
dc.description.abstract | Type Ic supernovae can be classified as normal supernovae Ic, type Ic super-luminous supernovae, X-ray flash-connected supernovae, broad-line supernovae Ic, and gamma-ray burst-connected supernovae. Here we suggest an inner connection for all kinds of supernovae Ic which is based on whether a pair of jets are successfully launched: a normal supernovae Ic is a normal core collapsar without jets launched; a gamma-ray burst-associated supernovae Ic is a core collapsar with relativistic jets launched and successfully breaking out the envelope of the progenitor; an X-ray flash-associated supernovae Ic is a core collapsar with jets launched but can only develop a relativistic shock breakout; a broad-line supernovae Ic is an off-axis gamma-ray burst or an X-ray flash-associated supernova; and a type Ic super-luminous supernovae is close to the X-ray flash-connected supernovae 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 supernovae Ic as a whole. We also show that the normal supernovae Ic and gamma-ray burst-connected supernovae Ic have similar accumulative distributions. | - |
dc.language | eng | - |
dc.publisher | Cambridge University Press. The Journal's web site is located at http://journals.cambridge.org/action/displayJournal?jid=pas | - |
dc.relation.ispartof | Publications of the Astronomical Society of Australia | - |
dc.rights | Publications of the Astronomical Society of Australia. Copyright © Cambridge University Press. | - |
dc.subject | Gamma-ray bursts | - |
dc.subject | Stars: evolution | - |
dc.subject | Stars: jets | - |
dc.subject | Stars: massive | - |
dc.subject | Supernovae | - |
dc.title | Toward an inner connection of SNe Ic, SLSNe Ic, XRF connected SNe, SNe Ic-BL, and GRB connected SNe | - |
dc.type | Article | - |
dc.identifier.email | Cheng, KS: hrspksc@hkucc.hku.hk | - |
dc.identifier.authority | Cheng, KS=rp00675 | - |
dc.description.nature | link_to_subscribed_fulltext | - |
dc.identifier.doi | 10.1017/pasa.2018.35 | - |
dc.identifier.scopus | eid_2-s2.0-85057420634 | - |
dc.identifier.hkuros | 296398 | - |
dc.identifier.volume | 35 | - |
dc.identifier.spage | article no. e032, p. 1 | - |
dc.identifier.epage | article no. e032, p. 8 | - |
dc.identifier.isi | WOS:000451029600001 | - |
dc.publisher.place | United Kingdom | - |
dc.identifier.issnl | 1323-3580 | - |