Multicolour polarization and CO observations towards a dark filament in Musca
Author:
Publisher
Oxford University Press (OUP)
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://academic.oup.com/mnras/article-pdf/265/1/1/2974492/mnras265-0001.pdf
Cited by 7 articles. 订阅此论文施引文献 订阅此论文施引文献,注册后可以免费订阅5篇论文的施引文献,订阅后可以查看论文全部施引文献
1. Distance, magnetic field, and kinematics of the filamentary cloud LDN 1157;Astronomy & Astrophysics;2020-07
2. Magnetic seismology of interstellar gas clouds: Unveiling a hidden dimension;Science;2018-05-11
3. Interplay of dust alignment, grain growth, and magnetic fields in polarization: lessons from the emission-to-extinction ratio;Astronomy & Astrophysics;2017-05-24
4. Properties of Dense Cores Embedded in Musca Derived from Extinction Maps and13CO, C18O, and NH3Emission Lines;The Astrophysical Journal;2017-02-06
5. The Musca cloud: A 6 pc-long velocity-coherent, sonic filament;Astronomy & Astrophysics;2016-02-24
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