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Table A.1:

Source properties and observational details.
Source Distance Luminosity Envelope Mass Type RA Dec Obs. Date Obs.id
  [pc] [$L_{\odot}$] [$M_{\odot}$]   [h m s] [ ${}^{\circ}~{\hbox{$^\prime$ }}~{\hbox{$^{\prime\prime}$ }}$]    
HH 46 450a 16b 5.1b Class I 08:25:43.9 -51:00:36 2009-10-26 1342186315 (PACS)
              2010-04-17 1342194783 (HIFI)
TMR 1 140c 3.7d 0.12e Class I 04:39:13.7 +25:53:21 2010-03-29 1342192984 (PACS)
IRAS 15398-3359 130f 0.92g 0.5h Class I 15:43:01.3 -34:09:15 2010-02-27 1342191302 (PACS)
DK Cha 178i 29.4j 0.03j Herbig Ae 12:53:17.2 -77:07:10.6 2009-12-10 1342188039 (PACS)
              2009-12-10 1342188040 (PACS)
NGC 7129 FIRS 2 1260k 500l 50m Intermed.-Mass 21:43:01.7 +66:03:23.6 2009-10-26 1342186321 (PACS)
NGC 1333 I 2A 235n 20o 1.0o Class 0 03:28:55.6 +31:14:37 2010-02-13 1342190686 (PACS)
              2010-02-24 1342191149 (PACS)
              2010-03-08 1342191773 (HIFI)
Serpens SMM1 415p 82.9q 8.7q Class 0     - ISOr
NGC 1333 I 4 235n 5.8o 4.5o Class 0     - ISOs

Notes. (a) Heathcote et al. (1996); (b) van Kempen et al. (2009a); (c) Motte et al. (1998); (d) Ohashi et al. (1996); (e) Jørgensen et al. (2002); (f) Murphy et al. (1986); (g) Froebrich (2005); (h) van Kempen et al. (2009b); (i) Whittet et al. (1997); (j) van Kempen et al. (2010a); (k) Shevchenko & Yakubov (1989); (l) Johnstone et al. (2010); (m) Crimier et al. (2010); (n) Hirota et al. (2008); (o) Jørgensen et al. (2009); (p) Dzib et al. (2010); (q) Hogerheijde et al. (1999) ( $L_{{\rm bol}}$ scaled to a distance of 415 pc); (r) Larsson et al. (2002); (s) Giannini et al. (2001).


Source LaTeX | All tables | In the text

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