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THE FILAMENTARY WEB OF STAR FORMATION

  • White, Glenn J. (Department of Physical Sciences, The Open University) ;
  • Doi, Yasuo (Department of Earth Science and Astronomy, the University of Tokyo) ;
  • Komugi, Shinya (Joint ALMA Observatory) ;
  • Kawada, Mitsunobu (Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency) ;
  • Takita, Satoshi (Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency) ;
  • Arimatsu, Ko (Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency) ;
  • Ikeda, Norio (Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency) ;
  • Kato, Daisuke (Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency) ;
  • Kitamura, Yoshimi (Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency) ;
  • Nakagawa, Takao (Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency) ;
  • Ootsubo, Takafumi (Astronomical Institute, Tohoku University) ;
  • Morishima, Takahiro (Astronomical Institute, Tohoku University) ;
  • Hattori, Makoto (Astronomical Institute, Tohoku University) ;
  • Tanaka, Masahiro (Center for Computational Sciences, University of Tsukuba) ;
  • Etxaluze, Mireya (Department of Physical Sciences, The Open University) ;
  • Shibai, Hiroshi (Department of Earth and Space Science, Osaka University)
  • Received : 2012.07.08
  • Accepted : 2012.07.25
  • Published : 2012.09.16

Abstract

Following the first Public Release of the AKARI Point Source catalogues, we have worked on the production of a new far-infrared All-Sky Diffuse mapping product. In this paper we report first results from the All Sky diffuse maps that will shortly be released to the community, based on analysis of data from the Far Infrared Surveyor ($65{\mu}m-160{\mu}m$) instrument. These data are likely to have a strong impact on studies of extended structures, and the diffuse ISM.

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