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ALMA view of the Galactic Center 50km/s molecular cloud

Published online by Cambridge University Press:  09 February 2017

Kenta Uehara
Affiliation:
Department of Astronomy, The University of Tokyo, Bunkyo, Tokyo 113-0033, Japan email: [email protected]
Masato Tsuboi
Affiliation:
Institute of Space and Astronautical Science, JAXA, Sagamihara, Kanagawa 252-5210, Japan
Yoshimi Kitamura
Affiliation:
Institute of Space and Astronautical Science, JAXA, Sagamihara, Kanagawa 252-5210, Japan
Ryosuke Miyawaki
Affiliation:
Colledge of Arts and Sciences, J.F. Oberlin University, Machida, Tokyo 194-0294, Japan
Atsushi Miyazaki
Affiliation:
Japan Space Forum, 3-2-1, Kandasurugadai, Chiyoda-ku, Tokyo 101-0062Japan
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Abstract

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We have observed the Galactic Center 50km/s molecular cloud (50MC) with ALMA to search for filamentary structures. In the CS J=2-1 emission line channel maps, we succeeded in identifying 27 molecular cloud filaments using the DisPerSE algorithm. This is the first attempt of filament-finding in the Galactic Center Region. These molecular cloud filaments strongly suggest that the molecular cloud filaments are also ubiquitous in the molecular clouds of the Galactic Center Region.

Type
Contributed Papers
Copyright
Copyright © International Astronomical Union 2017 

References

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