Morphokinematic properties of the 21 micron source IRAS 22272+5435
Jun‐ichi Nakashima, Sun Kwok, Bosco H. K. Yung, Yong Zhang, Nico Koning, N. H. Volgenau
Abstract
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Jun‐ichi Nakashima, Sun Kwok, Bosco H. K. Yung, Yong Zhang, Nico Koning, N. H. Volgenau
Abstract
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Abstract We obtained a high-resolution CO map of IRAS 22272+5435 in the CO J = 2–1 line using CARMA. The target exhibits a second biggest angular size of the circumstellar molecular envelope among known 21 μm sources. In the preliminary results, we found that the CO properties of IRAS 22272+5435 is clearly different from those of IRAS 07134+1005, which is another well-investigated 21 μm source. For example, elongations seen in the mid-infrared and CO images are extended in mutually perpendicular directions, although in case of IRAS 07134+1005 the CO feature coincides well with the mid-infrared structure.
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Abstract We obtained a high-resolution CO map of IRAS 22272+5435 in the CO J = 2–1 line using CARMA. The target exhibits a second biggest angular size of the circumstellar molecular envelope among known 21 μm sources. In the preliminary results, we found that the CO properties of IRAS 22272+5435 is clearly different from those of IRAS 07134+1005, which is another well-investigated 21 μm source. For example, elongations seen in the mid-infrared and CO images are extended in mutually perpendicular directions, although in case of IRAS 07134+1005 the CO feature coincides well with the mid-infrared structure.
Key concepts: Envelope (radar), Perpendicular, Circumstellar envelope, Physics, Line (geometry), Infrared, Astrophysics, Angular resolution (graph drawing)