Matches in SemOpenAlex for { <https://semopenalex.org/work/W3124139557> ?p ?o ?g. }
- W3124139557 endingPage "1464" @default.
- W3124139557 startingPage "1455" @default.
- W3124139557 abstract "We construct a parameterized model to explore the main properties of the star formation history of M33. We assume that the disk originates and grows by the primordial gas infall and adopt the simple form of gas accretion rate with one free parameter, the infall time-scale. We also include the contribution of gas outflow process. A major update of the model is that we adopt a molecular hydrogen correlated star formation law and calculate the evolution of the atomic and molecular gas separately. Comparisons between the model predictions and the observational data show that the model predictions are very sensitive to the adopted infall time-scale, while the gas outflow process mainly influences the metallicity profile. The model adopting a moderate outflow rate and an inside-out formation scenario can be in good agreement with most of observed constraints of M33 disk. We also compare the model predictions based on the molecular hydrogen correlated star formation law and that based on the Kennicutt star formation law. Our results imply that the molecular hydrogen correlated star formation law should be preferred to describe the evolution of the M33 disk, especially the radial distributions of both the cold gas and the stellar population." @default.
- W3124139557 created "2021-02-01" @default.
- W3124139557 creator A5024822458 @default.
- W3124139557 creator A5034116363 @default.
- W3124139557 creator A5044194134 @default.
- W3124139557 creator A5057340137 @default.
- W3124139557 creator A5071773009 @default.
- W3124139557 creator A5077456863 @default.
- W3124139557 creator A5088362654 @default.
- W3124139557 date "2012-10-01" @default.
- W3124139557 modified "2023-09-23" @default.
- W3124139557 title "The evolution and star-formation history of M33" @default.
- W3124139557 cites W1967083473 @default.
- W3124139557 cites W1970660289 @default.
- W3124139557 cites W1982017213 @default.
- W3124139557 cites W1984555273 @default.
- W3124139557 cites W1986285204 @default.
- W3124139557 cites W1988790306 @default.
- W3124139557 cites W1989718437 @default.
- W3124139557 cites W1994515292 @default.
- W3124139557 cites W1994671833 @default.
- W3124139557 cites W1997272299 @default.
- W3124139557 cites W2004118815 @default.
- W3124139557 cites W2006813182 @default.
- W3124139557 cites W2006878995 @default.
- W3124139557 cites W2006958273 @default.
- W3124139557 cites W2007275578 @default.
- W3124139557 cites W2012919097 @default.
- W3124139557 cites W2016759553 @default.
- W3124139557 cites W2016847354 @default.
- W3124139557 cites W2017364885 @default.
- W3124139557 cites W2030579627 @default.
- W3124139557 cites W2032471326 @default.
- W3124139557 cites W2035225065 @default.
- W3124139557 cites W2036750183 @default.
- W3124139557 cites W2036880118 @default.
- W3124139557 cites W2040322225 @default.
- W3124139557 cites W2041151710 @default.
- W3124139557 cites W2041253969 @default.
- W3124139557 cites W2042738789 @default.
- W3124139557 cites W2047657969 @default.
- W3124139557 cites W2049300959 @default.
- W3124139557 cites W2051920470 @default.
- W3124139557 cites W2054318713 @default.
- W3124139557 cites W2055518619 @default.
- W3124139557 cites W2058019727 @default.
- W3124139557 cites W2058889425 @default.
- W3124139557 cites W2062961789 @default.
- W3124139557 cites W2067857092 @default.
- W3124139557 cites W2068967919 @default.
- W3124139557 cites W2081897809 @default.
- W3124139557 cites W2088536005 @default.
- W3124139557 cites W2116466430 @default.
- W3124139557 cites W2120031672 @default.
- W3124139557 cites W2123839551 @default.
- W3124139557 cites W2133064652 @default.
- W3124139557 cites W2134710691 @default.
- W3124139557 cites W2155593555 @default.
- W3124139557 cites W2155670397 @default.
- W3124139557 cites W2161449264 @default.
- W3124139557 cites W2161534098 @default.
- W3124139557 cites W2164266869 @default.
- W3124139557 cites W2165528988 @default.
- W3124139557 cites W2167240457 @default.
- W3124139557 cites W2168110081 @default.
- W3124139557 cites W2899497983 @default.
- W3124139557 cites W3098049141 @default.
- W3124139557 cites W3098197335 @default.
- W3124139557 cites W3099074238 @default.
- W3124139557 cites W3099132502 @default.
- W3124139557 cites W3100152050 @default.
- W3124139557 cites W3101940179 @default.
- W3124139557 cites W3103128599 @default.
- W3124139557 cites W3103977363 @default.
- W3124139557 cites W3104877273 @default.
- W3124139557 cites W3105013135 @default.
- W3124139557 cites W3105658094 @default.
- W3124139557 cites W3122503815 @default.
- W3124139557 cites W4301942467 @default.
- W3124139557 doi "https://doi.org/10.1111/j.1365-2966.2012.21778.x" @default.
- W3124139557 hasPublicationYear "2012" @default.
- W3124139557 type Work @default.
- W3124139557 sameAs 3124139557 @default.
- W3124139557 citedByCount "15" @default.
- W3124139557 countsByYear W31241395572012 @default.
- W3124139557 countsByYear W31241395572013 @default.
- W3124139557 countsByYear W31241395572014 @default.
- W3124139557 countsByYear W31241395572015 @default.
- W3124139557 countsByYear W31241395572016 @default.
- W3124139557 countsByYear W31241395572017 @default.
- W3124139557 countsByYear W31241395572018 @default.
- W3124139557 countsByYear W31241395572019 @default.
- W3124139557 countsByYear W31241395572021 @default.
- W3124139557 countsByYear W31241395572022 @default.
- W3124139557 crossrefType "journal-article" @default.
- W3124139557 hasAuthorship W3124139557A5024822458 @default.
- W3124139557 hasAuthorship W3124139557A5034116363 @default.
- W3124139557 hasAuthorship W3124139557A5044194134 @default.