S |Dist is SDist K |Dist is KDist SC |complex distance computed by averaging the stellar distances (SDist) of the member clusters KC |complex distance computed kinematically from an average position and velocity, using the values compiled here for all the clusters within the complex with available (and not repeated) Vlsr C(ID:157) |adopted for the whole complex the distance given for the cluster with ID = 157 C(ID:36) |adopted for the whole complex the distance given for the cluster with ID = 36 C(ID:76) |adopted for the whole complex the distance given for the cluster with ID = 76 C(ID:438) |adopted for the whole complex the distance given for the cluster with ID = 438 C(ID:473) |adopted for the whole complex the distance given for the cluster with ID = 473 C(ID:484) |adopted for the whole complex the distance given for the cluster with ID = 484 C(ID:525) |adopted for the whole complex the distance given for the cluster with ID = 525 C(ID:527) |adopted for the whole complex the distance given for the cluster with ID = 527 C(ID:534) |adopted for the whole complex the distance given for the cluster with ID = 534 C(ID:601) |adopted for the whole complex the distance given for the cluster with ID = 601 C(ID:604) |adopted for the whole complex the distance given for the cluster with ID = 604 C(ID:621) |adopted for the whole complex the distance given for the cluster with ID = 621 C(ID:657) |adopted for the whole complex the distance given for the cluster with ID = 657 C(ID:693) |adopted for the whole complex the distance given for the cluster with ID = 693 C(Ref:48) |distance for the whole complex adopted from 2011A&A...527A.141C Cambresy et al. C(Ref:153) |distance for the whole complex adopted from 1978A&A....69...51N Neckel C(Ref:222) |distance for the whole complex adopted from 2010MNRAS.407..923S Stead & Hoare C(Ref:257) |distance for the whole complex adopted from 2007A&A...472..835Z Zavagno et al. CV(Ref:9) |complex distance computed kinematically from an average position and velocity given by 2006MNRAS.367.1609B Bains et al. CV(Ref:131) |complex distance computed kinematically from an average position and velocity given by 2011A&A...534A.131L Lopez et al. CV(Ref:157) |complex distance computed kinematically from an average position and velocity given by 2011A&A...529A..41N Nguyen Luong et al. Ref:10 |2008A&A...490..787B Bartkiewicz et al. Ref:31 |1999ApJ...512..237B Blum & Damineli Ref:45 |2009ApJ...693..424B Brunthaler et al. Ref:95 |2010RvMP...82.3121G Genzel et al. Ref:99 |1992ApJ...393..149G Gwinn et al. Ref:111 |2011A&A...536A..48K Kainulainen et al. Ref:124 |2011PASJ...63..513K Kurayama et al. Ref:136 |2009ApJ...706..727M Marshall et al. Ref:150 |2011PASJ...63...31M Motogi et al. Ref:152 |2011PASJ...63..719N Nagayama et al. Ref:159 |2010PASJ...62..101O Oh et al. Ref:192 |2009ApJ...700..137R Reid et al. Ref:212 |2010PASJ...62..287S Sato et al. Ref:213 |2010ApJ...720.1055S Sato et al. Ref:222 |2010MNRAS.407..923S Stead & Hoare Ref:252 |2008AJ....135..693W Wolk et al. Ref:254 |2009ApJ...693..413X Xu et al. Ref:255 |2011ApJ...733...25X Xu et al. Ref:258 |2009ApJ...693..419Z Zhang et al. 5 |2009ApJ...690..706A Anderson & Bania 5* |2009ApJ...690..706A Anderson & Bania, the source with resolved KDA is not the same as name_Vlsr, but is close in phase-space C |KDA solution for the whole associated complex, or from a particular source in the complex D |source associated with an IRDC, favoring the near distance O |out of the solar circle, i.e., no ambiguity in the kinematic distance S |adopted KDA solution consistent with the SDist z |far distance discarded because otherwise z>200pc above the Galactic plane (5) |2009ApJ...690..706A Anderson & Bania, contradicts the adopted KDA solution (7) |2008A&A...486..807A Arnal et al., contradicts the adopted KDA solution (D) |source associated with an IRDC, favoring the near distance and contradicts the adopted KDA solution 10* |2008A&A...490..787B Bartkiewicz et al., the source with resolved KDA is not the same as name_Vlsr, but is close in phase-space (44) |2008ApJ...672..391B Bronfman et al., contradicts the adopted KDA solution 45* |2009ApJ...693..424B Brunthaler et al., the source with resolved KDA is not the same as name_Vlsr, but is close in phase-space 51 | 1987A&A...171..261C Caswell & Haynes 51* | 1987A&A...171..261C Caswell & Haynes, the source with resolved KDA is not the same as name_Vlsr, but is close in phase-space (51) | 1987A&A...171..261C Caswell & Haynes, contradicts the adopted KDA solution (51*) | 1987A&A...171..261C Caswell & Haynes, contradicts the adopted KDA solution and the source with resolved KDA is not the same as name_Vlsr, but is close in phase-space 54 | 1990A&AS...83..119C Churchwell et al. 71 |2010A&A...523A...6D Deharveng et al. 72 | 1980A&AS...40..379D Downes et al. (72) | 1980A&AS...40..379D Downes et al., contradicts the adopted KDA solution 75 |2004A&A...426...97F Faundez et al. 75* |2004A&A...426...97F Faundez et al., the source with resolved KDA is not the same as name_Vlsr, but is close in phase-space (75) |2004A&A...426...97F Faundez et al., contradicts the adopted KDA solution 90 |2007ApJ...666..309G Garay et al. 92 | 1987A&A...174..257G Georgelin et al. (92) | 1987A&A...174..257G Georgelin et al., contradicts the adopted KDA solution 93 | 1994A&AS..108..513G Georgelin et al. 94 | 1996A&AS..120...41G Georgelin et al. 94* | 1996A&AS..120...41G Georgelin et al., the source with resolved KDA is not the same as name_Vlsr, but is close in phase-space 97 | 1990A&A...234..447G Gomez et al. 98 |2011MNRAS.417.2500G Green & McClure-Griffiths (98) |2011MNRAS.417.2500G Green & McClure-Griffiths, contradicts the adopted KDA solution 99 | 1992ApJ...393..149G Gwinn et al. 108 |2008ApJ...680..349J Jackson et al. 110 |2009ApJ...707..283J Johnston et al. 111 |2011A&A...536A..48K Kainulainen et al. 119 |2003ApJ...582..756K Kolpak et al. 121 |2007A&A...468..993K Kothes & Dougherty 124 |2011PASJ...63..513K Kurayama et al. 136 |2009ApJ...706..727M Marshall et al. 149 | 1996A&A...308..573M Molinari et al. (149) | 1996A&A...308..573M Molinari et al., contradicts the adopted KDA solution 150* |2011PASJ...63...31M Motogi et al., the source with resolved KDA is not the same as name_Vlsr, but is close in phase-space 159 |2010PASJ...62..101O Oh et al. 162 |2008A&A...486..191P Pandian et al. (162) |2008A&A...486..191P Pandian et al., contradicts the adopted KDA solution (162*) |2008A&A...486..191P Pandian et al., contradicts the adopted KDA solution and the source with resolved KDA is not the same as name_Vlsr, but is close in phase-space 163 |2009ApJ...706.1609P Pandian et al. (163) |2009ApJ...706.1609P Pandian et al., contradicts the adopted KDA solution 186 |2006MNRAS.367..553P Purcell et al. 187 |2008ASPC..387..381U Urquhart et al. 187* |2008ASPC..387..381U Urquhart et al., the source with resolved KDA is not the same as name_Vlsr, but is close in phase-space (187) |2008ASPC..387..381U Urquhart et al., contradicts the adopted KDA solution (187*) |2008ASPC..387..381U Urquhart et al., contradicts the adopted KDA solution and the source with resolved KDA is not the same as name_Vlsr, but is close in phase-space 195 |2009ApJ...699.1153R Roman-Duval et al. 195* |2009ApJ...699.1153R Roman-Duval et al., the source with resolved KDA is not the same as name_Vlsr, but is close in phase-space (195) |2009ApJ...699.1153R Roman-Duval et al., contradicts the adopted KDA solution 204 |2003A&A...397..133R Russeil 204* |2003A&A...397..133R Russeil, the source with resolved KDA is not the same as name_Vlsr, but is close in phase-space 206 |2005A&A...429..497R Russeil et al. 206* |2005A&A...429..497R Russeil et al., the source with resolved KDA is not the same as name_Vlsr, but is close in phase-space (206) |2005A&A...429..497R Russeil et al., contradicts the adopted KDA solution 212 |2010PASJ...62..287S Sato et al. 216 |2004ApJS..154..553S Sewilo et al. (216) |2004ApJS..154..553S Sewilo et al., contradicts the adopted KDA solution 222 |2010MNRAS.407..923S Stead & Hoare 222* |2010MNRAS.407..923S Stead & Hoare, the source with resolved KDA is not the same as name_Vlsr, but is close in phase-space 224 | 1982ApJS...48..127S Stier et al. 239* |2012MNRAS.420.1656U Urquhart et al., the source with resolved KDA is not the same as name_Vlsr, but is close in phase-space 254 |2009ApJ...693..413X Xu et al. 255 |2011ApJ...733...25X Xu et al. 258 |2009ApJ...693..419Z Zhang et al.