【作者单位】National Astronomical Observatories, Chinese Academy of Sciences, Beijing 100101, China;CAS Key Laboratory of FAST, National Astronomical Observatories, Chinese Academy of Sciences, Beijing 100101, China;NAOC-TU Joint Center for Astrophysics, Lhasa 850000, China;I. Physikalisches Institut, Universitt zu Kln, Zülpicher Str. 77, 50937 Kln, Germany;Department of Astronomy, Peking University, Beijing 100871, China;National Astronomical Observatories, Chinese Academy of Sciences, Beijing 100101, China;CAS Key Laboratory of FAST, National Astronomical Observatories, Chinese Academy of Sciences, Beijing 100101, China;NAOC-TU Joint Center for Astrophysics, Lhasa 850000, China;National Astronomical Observatories, Chinese Academy of Sciences, Beijing 100101, China;CAS Key Laboratory of FAST, National Astronomical Observatories, Chinese Academy of Sciences, Beijing 100101, China;NAOC-TU Joint Center for Astrophysics, Lhasa 850000, China;I. Physikalisches Institut, Universitt zu Kln, Zülpicher Str. 77, 50937 Kln, Germany;School of Astronomy and Space Science, Nanjing University, Nanjing 210023, China;Department of Astronomy, Yunnan University, and Key Laboratory of Astroparticle Physics of Yunnan Province, Kunming 650091, China;Shanghai Astronomical Observatory, Chinese Academy of Sciences, Shanghai 200030, China;Tibet University, Lhasa, Tibet 850000, China;NAOC-TU Joint Center for Astrophysics, Lhasa 850000, China;Tibet University, Lhasa, Tibet 850000, China;NAOC-TU Joint Center for Astrophysics, Lhasa 850000, China;Tibet University, Lhasa, Tibet 850000, China;NAOC-TU Joint Center for Astrophysics, Lhasa 850000, China;National Astronomical Observatories, Chinese Academy of Sciences, Beijing 100101, China;CAS Key Laboratory of FAST, National Astronomical Observatories, Chinese Academy of Sciences, Beijing 100101, China;NAOC-TU Joint Center for Astrophysics, Lhasa 850000, China;National Astronomical Observatories, Chinese Academy of Sciences, Beijing 100101, China;NAOC-TU Joint Center for Astrophysics, Lhasa 850000, China;National Astronomical Observatories, Chinese Academy of Sciences, Beijing 100101, China;NAOC-TU Joint Center for Astrophysics, Lhasa 850000, China;National Astronomical Observatories, Chinese Academy of Sciences, Beijing 100101, China;CAS Key Laboratory of FAST, National Astronomical Observatories, Chinese Academy of Sciences, Beijing 100101, China;NAOC-TU Joint Center for Astrophysics, Lhasa 850000, China;I. Physikalisches Institut, Universitt zu Kln, Zülpicher Str. 77, 50937 Kln, Germany;I. Physikalisches Institut, Universitt zu Kln, Zülpicher Str. 77, 50937 Kln, Germany;National Astronomical Observatories, Chinese Academy of Sciences, Beijing 100101, China;CAS Key Laboratory of FAST, National Astronomical Observatories, Chinese Academy of Sciences, Beijing 100101, China;NAOC-TU Joint Center for Astrophysics, Lhasa 850000, China;National Astronomical Observatories, Chinese Academy of Sciences, Beijing 100101, China;NAOC-TU Joint Center for Astrophysics, Lhasa 850000, China;National Astronomical Observatories, Chinese Academy of Sciences, Beijing 100101, China;NAOC-TU Joint Center for Astrophysics, Lhasa 850000, China;Tibet University, Lhasa, Tibet 850000, China;NAOC-TU Joint Center for Astrophysics, Lhasa 850000, China
【年份】2019
【卷号】Vol.19 No.12
【页码】183
【ISSN】1674-4527;2397-6209
【摘要】 We have performed a multi-wavelength study toward a quasi-sinusoidal filament (CFG028.68–0.28). A new large-scale 12 CO J = 3 – 2 map was obtained from the China-Cologne Observation for SubMillimeter Astronomy (CCOSMA) 3m radio telescope. Based on t...
