FRINK Linked Data Fragments server

Matches in SemOpenAlex for { <https://semopenalex.org/work/W3099214327> ?p ?o ?g. }

• W3099214327 endingPage "41" @default.
• W3099214327 startingPage "41" @default.
• W3099214327 abstract "Recent high-cadence transient surveys and rapid follow-up observations indicate that some massive stars may dynamically lose their own mass within decades before supernovae (SNe). Such a mass-loss forms `confined' circumstellar medium (CSM); a high density material distributed only within a small radius ($lesssim 10^{15}$ cm with the mass-loss rate of 0.01 $sim 10^{-4} M_odot$ yr$^{-1}$). While the SN shock should trigger particle acceleration and magnetic field amplification in the `confined' CSM, synchrotron emission may be masked in centimeter wavelengths due to free-free absorption; the millimeter range can however be a potential new window. We investigate the time evolution of synchrotron radiation from the system of a red super giant surrounded by the `confined' CSM, relevant to typical type II-P SNe. We show that synchrotron millimeter emission is generally detectable, and the signal can be used as a sensitive tracer of the nature of the `confined' CSM; it traces different CSM density parameter space than in the optical. Furthermore, our simulations show that the `confined' CSM efficiently produces secondary electrons and positrons through proton inelastic collisions, which can become main contributors to the synchrotron emission in several ten days since the SN. We predict that the synchrotron emission is detectable by ALMA, and suggest that it will provide a robust evidence of the existence of the `confined' CSM." @default.
• W3099214327 created "2020-11-23" @default.
• W3099214327 creator A5032359774 @default.
• W3099214327 creator A5041375615 @default.
• W3099214327 creator A5064897101 @default.
• W3099214327 creator A5090448677 @default.
• W3099214327 date "2019-10-29" @default.
• W3099214327 modified "2023-09-27" @default.
• W3099214327 title "Radio Emission from Supernovae in the Very Early Phase: Implications for the Dynamical Mass Loss of Massive Stars" @default.
• W3099214327 cites W1982425667 @default.
• W3099214327 cites W1989756559 @default.
• W3099214327 cites W2000909045 @default.
• W3099214327 cites W2006124034 @default.
• W3099214327 cites W2006785706 @default.
• W3099214327 cites W2007030757 @default.
• W3099214327 cites W2011255110 @default.
• W3099214327 cites W2011634292 @default.
• W3099214327 cites W2028731326 @default.
• W3099214327 cites W2032754772 @default.
• W3099214327 cites W2040051355 @default.
• W3099214327 cites W2041766317 @default.
• W3099214327 cites W2042602321 @default.
• W3099214327 cites W2044626047 @default.
• W3099214327 cites W2064221922 @default.
• W3099214327 cites W2069926710 @default.
• W3099214327 cites W2072151606 @default.
• W3099214327 cites W2072362373 @default.
• W3099214327 cites W2073564169 @default.
• W3099214327 cites W2083217178 @default.
• W3099214327 cites W2096911128 @default.
• W3099214327 cites W2100867411 @default.
• W3099214327 cites W2140288612 @default.
• W3099214327 cites W2142542912 @default.
• W3099214327 cites W2154178173 @default.
• W3099214327 cites W2159538809 @default.
• W3099214327 cites W2161736691 @default.
• W3099214327 cites W2170070152 @default.
• W3099214327 cites W2184731198 @default.
• W3099214327 cites W2290790711 @default.
• W3099214327 cites W2542640601 @default.
• W3099214327 cites W2579264406 @default.
• W3099214327 cites W2581714195 @default.
• W3099214327 cites W2609485152 @default.
• W3099214327 cites W2611048712 @default.
• W3099214327 cites W2767058944 @default.
• W3099214327 cites W2810798549 @default.
• W3099214327 cites W2889232959 @default.
• W3099214327 cites W2905450617 @default.
• W3099214327 cites W2911890654 @default.
• W3099214327 cites W2923877290 @default.
• W3099214327 cites W2963716729 @default.
• W3099214327 cites W3097976388 @default.
• W3099214327 cites W3099632739 @default.
• W3099214327 cites W3100131885 @default.
• W3099214327 cites W3100743249 @default.
• W3099214327 cites W3101687685 @default.
• W3099214327 cites W3103120247 @default.
• W3099214327 cites W3103999057 @default.
• W3099214327 cites W3105379451 @default.
• W3099214327 cites W3125562454 @default.
• W3099214327 cites W337816440 @default.
• W3099214327 cites W4297956063 @default.
• W3099214327 doi "https://doi.org/10.3847/1538-4357/ab4421" @default.
• W3099214327 hasPublicationYear "2019" @default.
• W3099214327 type Work @default.
• W3099214327 sameAs 3099214327 @default.
• W3099214327 citedByCount "10" @default.
• W3099214327 countsByYear W30992143272020 @default.
• W3099214327 countsByYear W30992143272021 @default.
• W3099214327 countsByYear W30992143272022 @default.
• W3099214327 countsByYear W30992143272023 @default.
• W3099214327 crossrefType "journal-article" @default.
• W3099214327 hasAuthorship W3099214327A5032359774 @default.
• W3099214327 hasAuthorship W3099214327A5041375615 @default.
• W3099214327 hasAuthorship W3099214327A5064897101 @default.
• W3099214327 hasAuthorship W3099214327A5090448677 @default.
• W3099214327 hasBestOaLocation W30992143271 @default.
• W3099214327 hasConcept C109792285 @default.
• W3099214327 hasConcept C121332964 @default.
• W3099214327 hasConcept C127592171 @default.
• W3099214327 hasConcept C1276947 @default.
• W3099214327 hasConcept C147120987 @default.
• W3099214327 hasConcept C150846664 @default.
• W3099214327 hasConcept C16332341 @default.
• W3099214327 hasConcept C178635117 @default.
• W3099214327 hasConcept C185544564 @default.
• W3099214327 hasConcept C21368211 @default.
• W3099214327 hasConcept C38652104 @default.
• W3099214327 hasConcept C41008148 @default.
• W3099214327 hasConcept C44870925 @default.
• W3099214327 hasConceptScore W3099214327C109792285 @default.
• W3099214327 hasConceptScore W3099214327C121332964 @default.
• W3099214327 hasConceptScore W3099214327C127592171 @default.
• W3099214327 hasConceptScore W3099214327C1276947 @default.
• W3099214327 hasConceptScore W3099214327C147120987 @default.
• W3099214327 hasConceptScore W3099214327C150846664 @default.
• W3099214327 hasConceptScore W3099214327C16332341 @default.
• W3099214327 hasConceptScore W3099214327C178635117 @default.

• next