Matches in SemOpenAlex for { <https://semopenalex.org/work/W2290576280> ?p ?o ?g. }
- W2290576280 endingPage "1392" @default.
- W2290576280 startingPage "1385" @default.
- W2290576280 abstract "Galaxy evolution is regulated by the interplay between galactic disks and their surrounding medium. We study this interplay by examining how the galactic coronal emission efficiency of stellar feedback depends on the (surface and specific) star formation rates (SFRs) and other parameters for a sample of 52 Chandra-observed nearby highly inclined disk galaxies. We first measure the star forming galactic disk sizes, as well as the SFRs of these galaxies, using data from the Wide-Field Infrared Survey Explorer, and then show that 1) the specific 0.5-2~keV luminosity of the coronal emission correlates with the specific SFR in a {sl sub-linear} fashion: on average, $L_X/L_K propto (SFR/M_*)^{Gamma}$ with $Gamma =0.29pm0.12$; 2) the efficiency of the emission $ L_X/SFR$ decreases with increasing surface SFR ($I_{SFR}$; $Gamma = -0.44pm0.12$); and 3) the characteristic temperature of the X-ray-emitting plasma weakly correlates with $I_{SFR}$ ($Gamma = 0.08pm0.04$). These results, somewhat surprising and anti-intuitive, suggest that a) the linear correlation between $L_X$ and SFR, as commonly presented, is largely due to the correlation of these two parameters with galaxy mass; b) much of the mechanical energy from stellar feedback likely drives global outflows with little X-ray cooling and with a mass-loading efficiency decreasing fast with increasing $I_{SFR}$ ($Gamma lesssim -0.5$); c) these outflows heat and inflate the medium around the galactic disks of massive galaxies, reducing its radiative cooling rate, whereas for relatively low-mass galaxies, the energy in the outflows is probably dissipated in regions far away from the galactic disks." @default.
- W2290576280 created "2016-06-24" @default.
- W2290576280 creator A5041296945 @default.
- W2290576280 creator A5061216377 @default.
- W2290576280 creator A5063077307 @default.
- W2290576280 creator A5064996219 @default.
- W2290576280 date "2016-02-04" @default.
- W2290576280 modified "2023-10-13" @default.
- W2290576280 title "<i>Chandra</i>survey of nearby highly inclined disk galaxies – IV. New insights into the working of stellar feedback" @default.
- W2290576280 cites W1494951942 @default.
- W2290576280 cites W1826320254 @default.
- W2290576280 cites W1860174610 @default.
- W2290576280 cites W1864729179 @default.
- W2290576280 cites W1889917103 @default.
- W2290576280 cites W1894826066 @default.
- W2290576280 cites W1898419174 @default.
- W2290576280 cites W1905835478 @default.
- W2290576280 cites W1920021936 @default.
- W2290576280 cites W1955162797 @default.
- W2290576280 cites W1964055719 @default.
- W2290576280 cites W1968491582 @default.
- W2290576280 cites W1983473287 @default.
- W2290576280 cites W1987635305 @default.
- W2290576280 cites W2001085255 @default.
- W2290576280 cites W2009693913 @default.
- W2290576280 cites W2011683230 @default.
- W2290576280 cites W2012220297 @default.
- W2290576280 cites W2012886609 @default.
- W2290576280 cites W2024011674 @default.
- W2290576280 cites W2028827636 @default.
- W2290576280 cites W2035467611 @default.
- W2290576280 cites W2044203116 @default.
- W2290576280 cites W2044509713 @default.
- W2290576280 cites W2046275384 @default.
- W2290576280 cites W2049782901 @default.
- W2290576280 cites W2052937506 @default.
- W2290576280 cites W2062113201 @default.
- W2290576280 cites W2076246932 @default.
- W2290576280 cites W2082092875 @default.
- W2290576280 cites W2083757268 @default.
- W2290576280 cites W2090675425 @default.
- W2290576280 cites W2106837094 @default.
- W2290576280 cites W2115496477 @default.
- W2290576280 cites W2115671411 @default.
- W2290576280 cites W2118920170 @default.
- W2290576280 cites W2120528046 @default.
- W2290576280 cites W2121247134 @default.
- W2290576280 cites W2124629497 @default.
- W2290576280 cites W2137239929 @default.
- W2290576280 cites W2140848834 @default.
- W2290576280 cites W2150035746 @default.
- W2290576280 cites W2154783802 @default.
- W2290576280 cites W2156709532 @default.
- W2290576280 cites W2159668413 @default.
- W2290576280 cites W2166365370 @default.
- W2290576280 cites W2169439142 @default.
- W2290576280 cites W2276719495 @default.
- W2290576280 cites W2323377960 @default.
- W2290576280 cites W3098784102 @default.
- W2290576280 cites W3099340296 @default.
- W2290576280 cites W3099361588 @default.
- W2290576280 cites W3099437765 @default.
- W2290576280 cites W3099739568 @default.
- W2290576280 cites W3099762132 @default.
- W2290576280 cites W3100007886 @default.
- W2290576280 cites W3100391850 @default.
- W2290576280 cites W3100840462 @default.
- W2290576280 cites W3102293467 @default.
- W2290576280 cites W3103105209 @default.
- W2290576280 cites W3103726718 @default.
- W2290576280 cites W3104818616 @default.
- W2290576280 cites W3105040958 @default.
- W2290576280 cites W3106265194 @default.
- W2290576280 cites W3106519446 @default.
- W2290576280 cites W3122040702 @default.
- W2290576280 cites W3123305420 @default.
- W2290576280 cites W4298195372 @default.
- W2290576280 cites W887389825 @default.
- W2290576280 doi "https://doi.org/10.1093/mnras/stv2886" @default.
- W2290576280 hasPublicationYear "2016" @default.
- W2290576280 type Work @default.
- W2290576280 sameAs 2290576280 @default.
- W2290576280 citedByCount "18" @default.
- W2290576280 countsByYear W22905762802016 @default.
- W2290576280 countsByYear W22905762802017 @default.
- W2290576280 countsByYear W22905762802018 @default.
- W2290576280 countsByYear W22905762802019 @default.
- W2290576280 countsByYear W22905762802020 @default.
- W2290576280 countsByYear W22905762802021 @default.
- W2290576280 countsByYear W22905762802022 @default.
- W2290576280 countsByYear W22905762802023 @default.
- W2290576280 crossrefType "journal-article" @default.
- W2290576280 hasAuthorship W2290576280A5041296945 @default.
- W2290576280 hasAuthorship W2290576280A5061216377 @default.
- W2290576280 hasAuthorship W2290576280A5063077307 @default.
- W2290576280 hasAuthorship W2290576280A5064996219 @default.
- W2290576280 hasBestOaLocation W22905762801 @default.
- W2290576280 hasConcept C121332964 @default.