LEADER 02178nam0 2200469 i 450 001 VAN0133419 005 20230619090412.846 017 70$2N$a9783662449691 100 $a20210412d2015 |0itac50 ba 101 $aeng 102 $aDE 105 $a|||| ||||| 200 1 $aˆThe ‰Earliest Stages of Massive Clustered Star Formation$eFragmentation of Infrared Dark Clouds$eDoctoral Thesis accepted by Peking University, Beijing, China$fKe Wang 210 $aBerlin$aHeidelberg$cSpringer$d2015 215 $axx, 145 p.$cill.$d24 cm 410 1$1001VAN0104193$12001 $aSpringer theses$erecognizing outstanding Ph.D. research$1210 $aBerlin$cSpringer$d2010- 500 1$3VAN0134226$aˆThe ‰Earliest Stages of Massive Clustered Star Formation$91771429 606 $a00A79 (77-XX)$xPhysics [MSC 2020]$3VANC023182$2MF 606 $a85-XX$xAstronomy and Astrophysics [MSC 2020]$3VANC023246$2MF 606 $a85A05$xGalactic and stellar dynamics [MSC 2020]$3VANC036147$2MF 610 $aGravitational Collapse and Fragmentation$9KW:K 610 $aHigh Angular Resolution$9KW:K 610 $aInfrared Dark Cloud$9KW:K 610 $aInterstellar Maser$9KW:K 610 $aInterstellar Medium$9KW:K 610 $aMassive Star Formation$9KW:K 610 $aProtostellar Jet and Outflow$9KW:K 610 $aRadio interferometers$9KW:K 610 $aSub Millimeter Array$9KW:K 610 $aVery Large Array$9KW:K 620 $dBerlin$3VANL000066 620 $aDE$dHeidelberg$3VANL000282 700 1$aWang$bKe$3VANV088762$0755911 712 $aSpringer $3VANV108073$4650 801 $aIT$bSOL$c20240614$gRICA 856 4 $uhttp://doi.org/10.1007/978-3-662-44969-1$zE-book ? Accesso al full-text attraverso riconoscimento IP di Ateneo, proxy e/o Shibboleth 899 $aBIBLIOTECA DEL DIPARTIMENTO DI MATEMATICA E FISICA$1IT-CE0120$2VAN08 912 $fN 912 $aVAN0133419 950 $aBIBLIOTECA DEL DIPARTIMENTO DI MATEMATICA E FISICA$d08CONS e-book 2255 $e08eMF2255 20210412 996 $aEarliest Stages of Massive Clustered Star Formation$91771429 997 $aUNICAMPANIA