LEADER 01515nam0 2200337 i 450 
001 SUN0133419
005 20210419122311.295
010   $d0.00
017 70$2N$a978-3-662-44969-1
100   $a20210412d2015       |0engc50      ba
101   $aeng
102   $aDE
105   $a||||    |||||
200 1 $aThe *Earliest Stages of Massive Clustered Star Formation$eFragmentation of Infrared Dark Clouds$eDoctoral Thesis accepted by Peking University, Beijing, China/ Ke Wang
205   $aBerlin$gHeidelberg : Springer, 2015
210   $axx$d145 p.$cill. ; 24 cm
215   $aPubblicazione in formato elettronico
410  1$1001SUN0104193$12001 $a*Springer theses$erecognizing outstanding Ph.D. research$1210  $aBerlin$aHeidelberg$cSpringer.
606   $a00A79 (77-XX)$xPhysics [MSC 2020]$2MF$3SUNC023182
606   $a85-XX$xAstronomy and Astrophysics [MSC 2020]$2MF$3SUNC023246
606   $a85A05$xGalactic and stellar dynamics [MSC 2020]$2MF$3SUNC036147
620   $dBerlin$3SUNL000066
620   $aDE$dHeidelberg$3SUNL000282
700  1$aWang$b, Ke$3SUNV088762$0755911
712   $aSpringer$3SUNV000178$4650
801   $aIT$bSOL$c20210426$gRICA
856 4 $uhttp://doi.org/10.1007/978-3-662-44969-1
912   $aSUN0133419
950   $aUFFICIO DI BIBLIOTECA DEL DIPARTIMENTO DI MATEMATICA E FISICA$d08CONS      e-book                  2255        $e08eMF2255              20210412            
996   $aEarliest Stages of Massive Clustered Star Formation$91771429
997   $aUNICAMPANIA