作者: Simon Gervais , Nicole St-Louis
DOI: 10.1086/301065
关键词: Local standard of rest 、 Position angle 、 Proper motion 、 Interstellar medium 、 Line-of-sight 、 Supersonic speed 、 Astronomy 、 Sky 、 Wolf–Rayet star 、 Astrophysics 、 Physics
摘要: Our H I maps reveal the existence of a nearly complete shell at velocity vsys = -11.44 km s-1 (Rs ≈ 20.9 pc, vexp 9.9 s-1, MH 1830 M⊙), which, mainly for morphological reasons, we associate with HD 191765 (although contribution from nearby W-R star 192103 cannot be totally excluded). The dynamical age this bubble (~1.3 × 106 yr) suggests that it was blown during main-sequence progenitor O-star phase. kinematic distance corresponding to local standard rest -11 is approximately 5 kpc, which incompatible association 2.1 kpc. Therefore, conclude have detected in gas already movement respect normal Galactic rotation region. There independent evidence present line sight. Recent Hipparcos data analyzed by Moffat et al. give supersonic proper motion (projected ~52 position angle on sky P.A. -38°). This vector points away very close center bubble, strengthens hypothesis physical link star. interstellar medium might generated some compression southwest region, rendering Hα brighter direction surroundings.