<?xml version="1.0" encoding="UTF-8"?><xml><records><record><source-app name="Biblio" version="7.x">Drupal-Biblio</source-app><ref-type>17</ref-type><contributors><authors><author><style face="normal" font="default" size="100%">Wang, K.</style></author><author><style face="normal" font="default" size="100%">Wu, Y. F.</style></author><author><style face="normal" font="default" size="100%">Ran, L.</style></author><author><style face="normal" font="default" size="100%">Yu, W. T.</style></author><author><style face="normal" font="default" size="100%">Miller, M.</style></author></authors></contributors><titles><title><style face="normal" font="default" size="100%">The relation between $^\13$\CO J = 2-1 line width in molecular clouds and bolometric luminosity of associated IRAS sources</style></title><secondary-title><style face="normal" font="default" size="100%">\aap</style></secondary-title></titles><keywords><keyword><style  face="normal" font="default" size="100%">Astrophysics - Solar and Stellar Astrophysics</style></keyword><keyword><style  face="normal" font="default" size="100%">ISM: clouds</style></keyword><keyword><style  face="normal" font="default" size="100%">ISM: kinematic and dynamics</style></keyword><keyword><style  face="normal" font="default" size="100%">ISM: molecules</style></keyword><keyword><style  face="normal" font="default" size="100%">stars: formation</style></keyword></keywords><dates><year><style  face="normal" font="default" size="100%">2009</style></year><pub-dates><date><style  face="normal" font="default" size="100%">nov</style></date></pub-dates></dates><number><style face="normal" font="default" size="100%">1</style></number><volume><style face="normal" font="default" size="100%">507</style></volume><pages><style face="normal" font="default" size="100%">369-376</style></pages><language><style face="normal" font="default" size="100%">eng</style></language></record></records></xml>