AKARI/FIS Mapping of the ISM-Wind Bow Shock around alpha Orionis

作者：Ueta Toshiya; Izumiura Hideyuki; Yamamura Issei; Nakada Yoshikazu; Matsuura Mikako; Ita Yoshifusa; Tanabe Toshihiko; Fukushi Hinako; Matsunaga Noriyuki; Mito Hiroyuki

来源：Publications of the Astronomical Society of Japan, 2008, 60: S407-S413.

• ISM: structure
• stars: individual (alpha Orionis)
• stars: kinematics
• stars: mass-loss
• stars: supergiants

We present 10' x 50'scan maps around an M supergiant alpha Ori at 65, 90, 140, and 160 mu m obtained with the AKARI Infrared Astronomy Satellite. Higher spatial resolution data with the exact analytic solution permit us to fit the de-projected shape of the stellar-wind bow shock around alpha Ori to have a stand-off distance of 4'.8, position angle of 55 degrees and inclination angle of 56 degrees. The shape of the bow shock suggests that the velocity of alpha Ori with respect to the local medium is upsilon(*) = 40n(H)(-1/2), where n(H) is the hydrogen nucleus density at alpha Ori. We found that the local medium is of n(H) = 1.5 to 1.9 cm(-3) and the velocity of the local flow is at 11 km s(-1) by using the most recent astrometric solutions for alpha Ori under the assumption that the medium local to alpha Ori is moving away from the Orion OB 1 association. AKARI images may also reveal a vortex ring due to instabilities on the surface of the bow shock, as demonstrated by numerical models. This research exemplifies the potential of AKARI All-Sky data as well as follow-up observations with Herschel Space Telescope and Stratospheric Observatory for Infrared Astronomy for this avenue of research in revealing the nature of the interaction between the stellar wind and the interstellar medium.

• 出版日期2008
• 单位中国科学院国家天文台