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Pattern analysis of young stellar clusters

Published online by Cambridge University Press:  21 March 2013

L. Viktor Tóth ,
Sarolta Zahorecz ,
Gábor Marton ,
Toshikazu Onishi ,
Lajos G. Balázs ,
Orsolya Fehér ,
Akiko Kawamura ,
Yoshimi Kitamura ,
Mónika Lisztes  and
Atsushi Nishimura
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L. Viktor Tóth
Affiliation:
Lorand Eotvos University, Department of Astronomy, Pazmany P.s. 1/a, 1117 Budapest, Hungary, email: l.v.toth@astro.elte.hu
Sarolta Zahorecz
Affiliation:
Lorand Eotvos University, Department of Astronomy, Pazmany P.s. 1/a, 1117 Budapest, Hungary, email: l.v.toth@astro.elte.hu
Gábor Marton
Affiliation:
Lorand Eotvos University, Department of Astronomy, Pazmany P.s. 1/a, 1117 Budapest, Hungary, email: l.v.toth@astro.elte.hu Konkoly Observatory of the Hungarian Ac. of Sci., PO Box 67, 1525 Budapest, Hungary
Toshikazu Onishi
Affiliation:
Department of Physical Science, Osaka Prefecture University, Gakuen 1-1, Sakai, Osaka 599-8531, Japan
Lajos G. Balázs
Affiliation:
Konkoly Observatory of the Hungarian Ac. of Sci., PO Box 67, 1525 Budapest, Hungary
Orsolya Fehér
Affiliation:
Lorand Eotvos University, Department of Astronomy, Pazmany P.s. 1/a, 1117 Budapest, Hungary, email: l.v.toth@astro.elte.hu
Akiko Kawamura
Affiliation:
National Astronomical Observatory of Japan, 2-21-1 Osawa, Mitaka, Tokyo 181-8588, Japan
Yoshimi Kitamura
Affiliation:
JAXA, 3-1-1 Yoshinodai, Sagamihara, Kanagawa, 229-8510, Japan
Mónika Lisztes
Affiliation:
Lorand Eotvos University, Department of Astronomy, Pazmany P.s. 1/a, 1117 Budapest, Hungary, email: l.v.toth@astro.elte.hu
Atsushi Nishimura
Affiliation:
Department of Physical Science, Osaka Prefecture University, Gakuen 1-1, Sakai, Osaka 599-8531, Japan
László Pásztor
Affiliation:
Research Institute for Soil Science and Agricultural Chemistry of the Hungarian Academy of Sciences, GIS Lab, Budapest, Hungary
Sándor Pintér
Affiliation:
Lorand Eotvos University, Department of Astronomy, Pazmany P.s. 1/a, 1117 Budapest, Hungary, email: l.v.toth@astro.elte.hu
Istvan Racz
Affiliation:
Lorand Eotvos University, Department of Astronomy, Pazmany P.s. 1/a, 1117 Budapest, Hungary, email: l.v.toth@astro.elte.hu
Motohide Tamura
Affiliation:
National Astronomical Observatory of Japan, 2-21-1 Osawa, Mitaka, Tokyo 181-8588, Japan
Munetaka Ueno
Affiliation:
JAXA, 3-1-1 Yoshinodai, Sagamihara, Kanagawa, 229-8510, Japan
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Abstract

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We revealed a statistically significant clustering in the all sky distribution of AKARI-WISE young stellar objects with large groups of elongated and bush types.

Keywords

stars: formation — ISM: individual (Orion molecular cloud complex)
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 8 , Symposium S292: Molecular Gas, Dust, and Star Formation in Galaxies , August 2012 , pp. 113
Copyright
Copyright © International Astronomical Union 2013

References

Cartwright, A., Whitworth, A. P. 2004, MNRAS, 348, 589CrossRefGoogle Scholar
Gutermuth, R. A.et al. 2009, ApJS, 184, 18Google Scholar
Tóth, L. V., Zahorecz, S., Marton, et al. 2012, in prep.Google Scholar
Wright, et al. 2010, AJ, 140, 1868Google Scholar
Yamamura, et al. 2010 AKARI/FIS All-Sky Survey Point Source Catalogues (ISAS/JAXA, 2010) PASJ, 59, 389Google Scholar