FRINK Linked Data Fragments server

Matches in SemOpenAlex for { <https://semopenalex.org/work/W4376866464> ?p ?o ?g. }

• W4376866464 endingPage "1440" @default.
• W4376866464 startingPage "1421" @default.
• W4376866464 abstract "Supernovae (SNe) inject $sim 10^{51}$ erg in the interstellar medium, thereby shocking and heating the gas. A substantial fraction of this energy is later lost via radiative cooling. We present a post-processing module for the FLASH code to calculate the cooling radiation from shock-heated gas using collisional excitation data from MAPPINGS V. When applying this tool to a simulated SN remnant (SNR), we find that most energy is emitted in the EUV. However, optical emission lines ($[$O III$]$, $[$N II$]$, $[$S II$]$, H${alpha}$, H${beta}$) are usually best observable. Our shock detection scheme shows that [S II] and [N II] emissions arise from the thin shell surrounding the SNR, while [O III], H$rm alpha$, and H$rm beta$ originate from the volume-filling hot gas inside the SNR bubble. We find that the optical emission lines are affected by the SNR's complex structure and its projection onto the plane of the sky because the escaping line luminosity can be reduced by 10 -- 80% due to absorption along the line-of-sight. Additionally, the subtraction of contaminating background radiation is required for the correct classification of an SNR on the oxygen or sulphur BPT diagrams. The electron temperature and density obtained from our synthetic observations match well with the simulation but are very sensitive to the assumed metallicity." @default.
• W4376866464 created "2023-05-18" @default.
• W4376866464 creator A5018273831 @default.
• W4376866464 creator A5022575311 @default.
• W4376866464 creator A5037317306 @default.
• W4376866464 creator A5038283208 @default.
• W4376866464 creator A5049542608 @default.
• W4376866464 creator A5078285187 @default.
• W4376866464 creator A5087614869 @default.
• W4376866464 date "2023-05-17" @default.
• W4376866464 modified "2023-09-23" @default.
• W4376866464 title "How do supernova remnants cool? – I. Morphology, optical emission lines, and shocks" @default.
• W4376866464 cites W1492690033 @default.
• W4376866464 cites W1498712972 @default.
• W4376866464 cites W1894745560 @default.
• W4376866464 cites W1967876247 @default.
• W4376866464 cites W1968945895 @default.
• W4376866464 cites W1969301376 @default.
• W4376866464 cites W1978574709 @default.
• W4376866464 cites W1989498628 @default.
• W4376866464 cites W1992741876 @default.
• W4376866464 cites W1993049583 @default.
• W4376866464 cites W1996905793 @default.
• W4376866464 cites W1999203878 @default.
• W4376866464 cites W2002447003 @default.
• W4376866464 cites W2002538061 @default.
• W4376866464 cites W2004597566 @default.
• W4376866464 cites W2005798315 @default.
• W4376866464 cites W2006391693 @default.
• W4376866464 cites W2009802717 @default.
• W4376866464 cites W2011301426 @default.
• W4376866464 cites W2014463822 @default.
• W4376866464 cites W2015999483 @default.
• W4376866464 cites W2025043891 @default.
• W4376866464 cites W2034608771 @default.
• W4376866464 cites W2037131602 @default.
• W4376866464 cites W2039241537 @default.
• W4376866464 cites W2048161484 @default.
• W4376866464 cites W2049052485 @default.
• W4376866464 cites W2051135785 @default.
• W4376866464 cites W2058468162 @default.
• W4376866464 cites W2062947338 @default.
• W4376866464 cites W2066255054 @default.
• W4376866464 cites W2067574896 @default.
• W4376866464 cites W2069887781 @default.
• W4376866464 cites W2070863847 @default.
• W4376866464 cites W2074130117 @default.
• W4376866464 cites W2079472587 @default.
• W4376866464 cites W2082092783 @default.
• W4376866464 cites W2085906808 @default.
• W4376866464 cites W2087597474 @default.
• W4376866464 cites W2088566550 @default.
• W4376866464 cites W2093807875 @default.
• W4376866464 cites W2095348844 @default.
• W4376866464 cites W2103056073 @default.
• W4376866464 cites W2108531802 @default.
• W4376866464 cites W2109510044 @default.
• W4376866464 cites W2112442951 @default.
• W4376866464 cites W2128036312 @default.
• W4376866464 cites W2133231861 @default.
• W4376866464 cites W2135026581 @default.
• W4376866464 cites W2138401193 @default.
• W4376866464 cites W2144418467 @default.
• W4376866464 cites W2153140383 @default.
• W4376866464 cites W2157917411 @default.
• W4376866464 cites W2163212281 @default.
• W4376866464 cites W2168006162 @default.
• W4376866464 cites W2236699209 @default.
• W4376866464 cites W2258178072 @default.
• W4376866464 cites W2335516212 @default.
• W4376866464 cites W2341424074 @default.
• W4376866464 cites W2443636255 @default.
• W4376866464 cites W2492135827 @default.
• W4376866464 cites W2496719331 @default.
• W4376866464 cites W2518701780 @default.
• W4376866464 cites W2543088168 @default.
• W4376866464 cites W2584823907 @default.
• W4376866464 cites W2608183658 @default.
• W4376866464 cites W2746808306 @default.
• W4376866464 cites W2756629902 @default.
• W4376866464 cites W2798807078 @default.
• W4376866464 cites W2886794481 @default.
• W4376866464 cites W2895966158 @default.
• W4376866464 cites W2899497983 @default.
• W4376866464 cites W2914645711 @default.
• W4376866464 cites W2919076651 @default.
• W4376866464 cites W2951323278 @default.
• W4376866464 cites W2969916546 @default.
• W4376866464 cites W2973159688 @default.
• W4376866464 cites W2985443361 @default.
• W4376866464 cites W3013636914 @default.
• W4376866464 cites W3043312982 @default.
• W4376866464 cites W3091725782 @default.
• W4376866464 cites W3094397837 @default.
• W4376866464 cites W3098385976 @default.
• W4376866464 cites W3098589636 @default.
• W4376866464 cites W3098784892 @default.
• W4376866464 cites W3098831132 @default.

• next