Classifying Maser features with Fortran and shell script for proper motion study of Water masers in W49N

• المؤلفون الرئيسيون: M. Phetra, K. Asanok, T. Hirota, B. H. Kramer, K. Sugiyama, W. Nuntiyakul
• التنسيق: وقائع المؤتمر
• منشور في: 2020
• الموضوعات: Physics and Astronomy
• الوصول للمادة أونلاين: https://www.scopus.com/inward/record.uri?partnerID=HzOxMe3b&scp=85077815933&origin=inward; http://cmuir.cmu.ac.th/jspui/handle/6653943832/68078
• المؤسسة: Chiang Mai University

© Published under licence by IOP Publishing Ltd. The 22-GHz Water masers in the W49N star-forming region are one of the richest and most luminous sources in our Galaxy, at the distance of 11.11 kpc. Very Long Baseline Interferometric (VLBI) observations allow us to study both physics of these masers...