<?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%">Xu, Xuefang</style></author><author><style face="normal" font="default" size="100%">Ke Wang</style></author><author><style face="normal" font="default" size="100%">Gou, Qian</style></author><author><style face="normal" font="default" size="100%">Baug, Tapas</style></author><author><style face="normal" font="default" size="100%">Di Li, Zhongshi Wang,</style></author><author><style face="normal" font="default" size="100%">Duan, Chunguo</style></author><author><style face="normal" font="default" size="100%">Lei, Juncheng</style></author></authors></contributors><titles><title><style face="normal" font="default" size="100%">The Milky Way atlas for linear filaments II. clump rotation versus filament orientation</style></title><secondary-title><style face="normal" font="default" size="100%">MNRAS</style></secondary-title></titles><keywords><keyword><style  face="normal" font="default" size="100%">Astrophysics - Astrophysics of Galaxies</style></keyword></keywords><dates><year><style  face="normal" font="default" size="100%">2024</style></year></dates><urls><web-urls><url><style face="normal" font="default" size="100%">https://academic.oup.com/mnras/advance-article/doi/10.1093/mnras/stae2379/7831688</style></url></web-urls></urls><volume><style face="normal" font="default" size="100%">535</style></volume><pages><style face="normal" font="default" size="100%">940</style></pages><language><style face="normal" font="default" size="100%">eng</style></language></record></records></xml>