Matches in SemOpenAlex for { <https://semopenalex.org/work/W3103141311> ?p ?o ?g. }
- W3103141311 endingPage "L93" @default.
- W3103141311 startingPage "L88" @default.
- W3103141311 abstract "We present a new high-resolution N-body/SPH simulation of an encounter of two gas-rich disk galaxies which closely matches the morphology and kinematics of the interacting Antennae galaxies (NGC 4038/39). The simulation includes radiative cooling, star formation and feedback from SNII. The large-scale morphology and kinematics are determined by the internal structure and the orbit of the progenitor disks. The properties of the central region, in particular the starburst in the overlap region, only match the observations for a very short time interval of ~20 Myr after the second encounter. This indicates that the Antennae galaxies are in a special phase only about 40 Myr after the second encounter and 50 Myr before their final collision. This is the only phase in the simulation when a gas-rich overlap region between the nuclei is forming accompanied by enhanced star formation. The star formation rate as well as the recent star formation history in the central region agree well with observational estimates. For the first time this new model explains the distributed extra-nuclear star formation in the Antennae galaxies as a consequence of the recent second encounter. The proposed model predicts that the Antennae are in a later merger stage than the Mice (NGC 4676) and would therefore lose their first place in the classical Toomre sequence." @default.
- W3103141311 created "2020-11-23" @default.
- W3103141311 creator A5022575311 @default.
- W3103141311 creator A5032012858 @default.
- W3103141311 creator A5033434486 @default.
- W3103141311 creator A5058218104 @default.
- W3103141311 creator A5084102989 @default.
- W3103141311 creator A5091283341 @default.
- W3103141311 creator A5029032425 @default.
- W3103141311 date "2010-05-05" @default.
- W3103141311 modified "2023-10-18" @default.
- W3103141311 title "ONE MOMENT IN TIME—MODELING STAR FORMATION IN THE ANTENNAE" @default.
- W3103141311 cites W1966727636 @default.
- W3103141311 cites W1973675768 @default.
- W3103141311 cites W1993324202 @default.
- W3103141311 cites W1993839984 @default.
- W3103141311 cites W1994968723 @default.
- W3103141311 cites W2007088574 @default.
- W3103141311 cites W2010598456 @default.
- W3103141311 cites W2011209242 @default.
- W3103141311 cites W2015994361 @default.
- W3103141311 cites W2028077189 @default.
- W3103141311 cites W2033357271 @default.
- W3103141311 cites W2040364743 @default.
- W3103141311 cites W2041542911 @default.
- W3103141311 cites W2046620005 @default.
- W3103141311 cites W2048602692 @default.
- W3103141311 cites W2060448616 @default.
- W3103141311 cites W2062369951 @default.
- W3103141311 cites W2065595147 @default.
- W3103141311 cites W2066886457 @default.
- W3103141311 cites W2067121603 @default.
- W3103141311 cites W2073879116 @default.
- W3103141311 cites W2080259687 @default.
- W3103141311 cites W2098564368 @default.
- W3103141311 cites W2099338922 @default.
- W3103141311 cites W2100514692 @default.
- W3103141311 cites W2100974914 @default.
- W3103141311 cites W2104393494 @default.
- W3103141311 cites W2114874982 @default.
- W3103141311 cites W2119572678 @default.
- W3103141311 cites W2134029361 @default.
- W3103141311 cites W2155225310 @default.
- W3103141311 cites W2170924363 @default.
- W3103141311 cites W3098221464 @default.
- W3103141311 cites W3098458856 @default.
- W3103141311 cites W3098845432 @default.
- W3103141311 cites W3100341808 @default.
- W3103141311 cites W3100380135 @default.
- W3103141311 cites W3100545852 @default.
- W3103141311 cites W3101352865 @default.
- W3103141311 cites W3101997500 @default.
- W3103141311 cites W3103375210 @default.
- W3103141311 cites W3103418232 @default.
- W3103141311 cites W3103899138 @default.
- W3103141311 cites W3105266433 @default.
- W3103141311 cites W3105575177 @default.
- W3103141311 cites W3105710181 @default.
- W3103141311 doi "https://doi.org/10.1088/2041-8205/715/2/l88" @default.
- W3103141311 hasPublicationYear "2010" @default.
- W3103141311 type Work @default.
- W3103141311 sameAs 3103141311 @default.
- W3103141311 citedByCount "65" @default.
- W3103141311 countsByYear W31031413112012 @default.
- W3103141311 countsByYear W31031413112013 @default.
- W3103141311 countsByYear W31031413112014 @default.
- W3103141311 countsByYear W31031413112015 @default.
- W3103141311 countsByYear W31031413112016 @default.
- W3103141311 countsByYear W31031413112017 @default.
- W3103141311 countsByYear W31031413112018 @default.
- W3103141311 countsByYear W31031413112019 @default.
- W3103141311 countsByYear W31031413112020 @default.
- W3103141311 countsByYear W31031413112021 @default.
- W3103141311 countsByYear W31031413112022 @default.
- W3103141311 countsByYear W31031413112023 @default.
- W3103141311 crossrefType "journal-article" @default.
- W3103141311 hasAuthorship W3103141311A5022575311 @default.
- W3103141311 hasAuthorship W3103141311A5029032425 @default.
- W3103141311 hasAuthorship W3103141311A5032012858 @default.
- W3103141311 hasAuthorship W3103141311A5033434486 @default.
- W3103141311 hasAuthorship W3103141311A5058218104 @default.
- W3103141311 hasAuthorship W3103141311A5084102989 @default.
- W3103141311 hasAuthorship W3103141311A5091283341 @default.
- W3103141311 hasBestOaLocation W31031413112 @default.
- W3103141311 hasConcept C104317684 @default.
- W3103141311 hasConcept C121332964 @default.
- W3103141311 hasConcept C125857072 @default.
- W3103141311 hasConcept C1276947 @default.
- W3103141311 hasConcept C141231307 @default.
- W3103141311 hasConcept C174802034 @default.
- W3103141311 hasConcept C185592680 @default.
- W3103141311 hasConcept C24389824 @default.
- W3103141311 hasConcept C2776401274 @default.
- W3103141311 hasConcept C39920418 @default.
- W3103141311 hasConcept C44870925 @default.
- W3103141311 hasConcept C55493867 @default.
- W3103141311 hasConcept C74650414 @default.
- W3103141311 hasConcept C98444146 @default.