FRINK Linked Data Fragments server

Matches in SemOpenAlex for { <https://semopenalex.org/work/W2011660810> ?p ?o ?g. }

• W2011660810 endingPage "1715" @default.
• W2011660810 startingPage "1703" @default.
• W2011660810 abstract "(Abridged) Heating of the interstellar medium by multiple supernovae (SNe) explosions is at the heart of producing galaxy-scale outflows. We use hydrodynamical simulations to study the efficiency of multiple SNe in heating the interstellar medium (ISM) and filling the volume with gas of high temperatures. We argue that it is important for SNe remnants to have a large filling factor {it and} a large heating efficiency. For this, they have to be clustered in space and time, and keep exploding until the hot gas percolates through the whole region, in order to compensate for the radiative loss. In the case of a limited number of SNe, we find that although the filling factor can be large, the heating efficiency declines after reaching a large value. In the case of a continuous series of SNe, the hot gas ($T ge 3 times 10^6$ K) can percolate through the whole region after the total volume filling factor reaches a threshold of $sim 0.3$. The efficiency of heating the gas to X-ray temperatures can be $ge 0.1$ after this percolation epoch, which occurs after a period of $approx 10$ Myr for a typical starburst SNe rate density of $nu_{rm SN} approx 10^{-9}$ pc$^{-3}$ yr$^{-1}$ and gas density of $napprox 10$ cm$^{-3}$ in starburst nuclei regions. This matches the recent observations of a time delay of similar order between the onset of star formation and galactic outflows. The efficiency to heat gas up to X-ray temperatures ($ge 10^{6.5}$ K) roughly scales as $nu_{rm SN}^{0.2} n^{-0.6}$. For a typical SNe rate density and gas density in starburst nuclei, the heating efficiency is $sim 0.15$, also consistent with previous interpretations from X-ray observations. We discuss the implications of our results with regard to observational diagnostics of ionic ratios and emission measures in starburst nuclei regions." @default.
• W2011660810 created "2016-06-24" @default.
• W2011660810 creator A5074432040 @default.
• W2011660810 creator A5076481155 @default.
• W2011660810 creator A5085140367 @default.
• W2011660810 date "2014-11-20" @default.
• W2011660810 modified "2023-09-24" @default.
• W2011660810 title "Evolution of multiple supernova remnants" @default.
• W2011660810 cites W1537224157 @default.
• W2011660810 cites W1918803940 @default.
• W2011660810 cites W1925826255 @default.
• W2011660810 cites W1939321231 @default.
• W2011660810 cites W1968695167 @default.
• W2011660810 cites W1969717379 @default.
• W2011660810 cites W1971043059 @default.
• W2011660810 cites W1975349204 @default.
• W2011660810 cites W1975983552 @default.
• W2011660810 cites W1994043696 @default.
• W2011660810 cites W1998182161 @default.
• W2011660810 cites W2004310296 @default.
• W2011660810 cites W2005106153 @default.
• W2011660810 cites W2009802717 @default.
• W2011660810 cites W2010689016 @default.
• W2011660810 cites W2012220297 @default.
• W2011660810 cites W2013997547 @default.
• W2011660810 cites W2014463822 @default.
• W2011660810 cites W2015980508 @default.
• W2011660810 cites W2018660153 @default.
• W2011660810 cites W2019602579 @default.
• W2011660810 cites W2028732061 @default.
• W2011660810 cites W2034485266 @default.
• W2011660810 cites W2035467611 @default.
• W2011660810 cites W2039241537 @default.
• W2011660810 cites W2049874509 @default.
• W2011660810 cites W2056918473 @default.
• W2011660810 cites W2061470180 @default.
• W2011660810 cites W2068928940 @default.
• W2011660810 cites W2069330501 @default.
• W2011660810 cites W2069887781 @default.
• W2011660810 cites W2088192313 @default.
• W2011660810 cites W2090675425 @default.
• W2011660810 cites W2091211628 @default.
• W2011660810 cites W2091990846 @default.
• W2011660810 cites W2094654900 @default.
• W2011660810 cites W2102792823 @default.
• W2011660810 cites W2154213758 @default.
• W2011660810 cites W2156030349 @default.
• W2011660810 cites W2159757668 @default.
• W2011660810 cites W2163746050 @default.
• W2011660810 cites W2168297633 @default.
• W2011660810 cites W2214031698 @default.
• W2011660810 cites W3099253078 @default.
• W2011660810 cites W3100391850 @default.
• W2011660810 cites W3100685835 @default.
• W2011660810 cites W3103949650 @default.
• W2011660810 cites W3123820624 @default.
• W2011660810 doi "https://doi.org/10.1093/mnras/stu2133" @default.
• W2011660810 hasPublicationYear "2014" @default.
• W2011660810 type Work @default.
• W2011660810 sameAs 2011660810 @default.
• W2011660810 citedByCount "29" @default.
• W2011660810 countsByYear W20116608102014 @default.
• W2011660810 countsByYear W20116608102015 @default.
• W2011660810 countsByYear W20116608102016 @default.
• W2011660810 countsByYear W20116608102017 @default.
• W2011660810 countsByYear W20116608102018 @default.
• W2011660810 countsByYear W20116608102019 @default.
• W2011660810 countsByYear W20116608102021 @default.
• W2011660810 countsByYear W20116608102022 @default.
• W2011660810 countsByYear W20116608102023 @default.
• W2011660810 crossrefType "journal-article" @default.
• W2011660810 hasAuthorship W2011660810A5074432040 @default.
• W2011660810 hasAuthorship W2011660810A5076481155 @default.
• W2011660810 hasAuthorship W2011660810A5085140367 @default.
• W2011660810 hasBestOaLocation W20116608101 @default.
• W2011660810 hasConcept C111919701 @default.
• W2011660810 hasConcept C121332964 @default.
• W2011660810 hasConcept C125857072 @default.
• W2011660810 hasConcept C127592171 @default.
• W2011660810 hasConcept C15908118 @default.
• W2011660810 hasConcept C196939603 @default.
• W2011660810 hasConcept C2777894999 @default.
• W2011660810 hasConcept C41008148 @default.
• W2011660810 hasConcept C44870925 @default.
• W2011660810 hasConcept C62520636 @default.
• W2011660810 hasConcept C74902906 @default.
• W2011660810 hasConcept C98444146 @default.
• W2011660810 hasConceptScore W2011660810C111919701 @default.
• W2011660810 hasConceptScore W2011660810C121332964 @default.
• W2011660810 hasConceptScore W2011660810C125857072 @default.
• W2011660810 hasConceptScore W2011660810C127592171 @default.
• W2011660810 hasConceptScore W2011660810C15908118 @default.
• W2011660810 hasConceptScore W2011660810C196939603 @default.
• W2011660810 hasConceptScore W2011660810C2777894999 @default.
• W2011660810 hasConceptScore W2011660810C41008148 @default.
• W2011660810 hasConceptScore W2011660810C44870925 @default.
• W2011660810 hasConceptScore W2011660810C62520636 @default.
• W2011660810 hasConceptScore W2011660810C74902906 @default.

• next