Matches in SemOpenAlex for { <https://semopenalex.org/work/W3100599046> ?p ?o ?g. }
- W3100599046 endingPage "115" @default.
- W3100599046 startingPage "115" @default.
- W3100599046 abstract "One puzzle in understanding how stars form in clusters is the source of mass -- is all of the mass in place before the first stars are born, or is there an extended period when the cluster accretes material which can continuously fuel the star formation process? We use a multi-line spectral survey of the southern filament associated with the Serpens South embedded cluster-forming region in order to determine if mass is accreting from the filament onto the cluster, and whether the accretion rate is significant. Our analysis suggests that material is flowing along the filament's long axis at a rate of ~30Msol/Myr (inferred from the N2H+ velocity gradient along the filament), and radially contracting onto the filament at ~130Msol/Myr (inferred from HNC self-absorption). These accretion rates are sufficient to supply mass to the central cluster at a similar rate to the current star formation rate in the cluster. Filamentary accretion flows may therefore be very important in the ongoing evolution of this cluster." @default.
- W3100599046 created "2020-11-23" @default.
- W3100599046 creator A5013062507 @default.
- W3100599046 creator A5022747856 @default.
- W3100599046 creator A5035126916 @default.
- W3100599046 creator A5046305273 @default.
- W3100599046 creator A5075144498 @default.
- W3100599046 creator A5082805955 @default.
- W3100599046 date "2013-03-15" @default.
- W3100599046 modified "2023-10-17" @default.
- W3100599046 title "FILAMENTARY ACCRETION FLOWS IN THE EMBEDDED SERPENS SOUTH PROTOCLUSTER" @default.
- W3100599046 cites W1502855581 @default.
- W3100599046 cites W1901242835 @default.
- W3100599046 cites W1924246703 @default.
- W3100599046 cites W1966062726 @default.
- W3100599046 cites W1983332987 @default.
- W3100599046 cites W1994742690 @default.
- W3100599046 cites W2002968199 @default.
- W3100599046 cites W2008579027 @default.
- W3100599046 cites W2010793265 @default.
- W3100599046 cites W2023055517 @default.
- W3100599046 cites W2041730224 @default.
- W3100599046 cites W2046580346 @default.
- W3100599046 cites W2050241132 @default.
- W3100599046 cites W2054594671 @default.
- W3100599046 cites W2054720561 @default.
- W3100599046 cites W2055506692 @default.
- W3100599046 cites W2064412245 @default.
- W3100599046 cites W2064528785 @default.
- W3100599046 cites W2081287082 @default.
- W3100599046 cites W2081652521 @default.
- W3100599046 cites W2085708302 @default.
- W3100599046 cites W2089176910 @default.
- W3100599046 cites W2092600640 @default.
- W3100599046 cites W2098683317 @default.
- W3100599046 cites W2101681357 @default.
- W3100599046 cites W2119766797 @default.
- W3100599046 cites W2121018712 @default.
- W3100599046 cites W2128294460 @default.
- W3100599046 cites W2132285486 @default.
- W3100599046 cites W2132926566 @default.
- W3100599046 cites W2138769428 @default.
- W3100599046 cites W2145822028 @default.
- W3100599046 cites W2154298686 @default.
- W3100599046 cites W2161424626 @default.
- W3100599046 cites W2162328595 @default.
- W3100599046 cites W3098276775 @default.
- W3100599046 cites W3098597880 @default.
- W3100599046 cites W3099015392 @default.
- W3100599046 cites W3099896119 @default.
- W3100599046 cites W3100015906 @default.
- W3100599046 cites W3100970929 @default.
- W3100599046 cites W3100976185 @default.
- W3100599046 cites W3101128596 @default.
- W3100599046 cites W3101351265 @default.
- W3100599046 cites W3102089187 @default.
- W3100599046 cites W3102127200 @default.
- W3100599046 cites W3102371208 @default.
- W3100599046 cites W3102728752 @default.
- W3100599046 cites W3104423841 @default.
- W3100599046 cites W3104805127 @default.
- W3100599046 cites W3105094438 @default.
- W3100599046 cites W3105280211 @default.
- W3100599046 cites W3105325670 @default.
- W3100599046 cites W4301347788 @default.
- W3100599046 doi "https://doi.org/10.1088/0004-637x/766/2/115" @default.
- W3100599046 hasPublicationYear "2013" @default.
- W3100599046 type Work @default.
- W3100599046 sameAs 3100599046 @default.
- W3100599046 citedByCount "225" @default.
- W3100599046 countsByYear W31005990462013 @default.
- W3100599046 countsByYear W31005990462014 @default.
- W3100599046 countsByYear W31005990462015 @default.
- W3100599046 countsByYear W31005990462016 @default.
- W3100599046 countsByYear W31005990462017 @default.
- W3100599046 countsByYear W31005990462018 @default.
- W3100599046 countsByYear W31005990462019 @default.
- W3100599046 countsByYear W31005990462020 @default.
- W3100599046 countsByYear W31005990462021 @default.
- W3100599046 countsByYear W31005990462022 @default.
- W3100599046 countsByYear W31005990462023 @default.
- W3100599046 crossrefType "journal-article" @default.
- W3100599046 hasAuthorship W3100599046A5013062507 @default.
- W3100599046 hasAuthorship W3100599046A5022747856 @default.
- W3100599046 hasAuthorship W3100599046A5035126916 @default.
- W3100599046 hasAuthorship W3100599046A5046305273 @default.
- W3100599046 hasAuthorship W3100599046A5075144498 @default.
- W3100599046 hasAuthorship W3100599046A5082805955 @default.
- W3100599046 hasBestOaLocation W31005990462 @default.
- W3100599046 hasConcept C121332964 @default.
- W3100599046 hasConcept C125857072 @default.
- W3100599046 hasConcept C1276947 @default.
- W3100599046 hasConcept C14228908 @default.
- W3100599046 hasConcept C150846664 @default.
- W3100599046 hasConcept C164866538 @default.
- W3100599046 hasConcept C168589115 @default.
- W3100599046 hasConcept C182276052 @default.
- W3100599046 hasConcept C199360897 @default.