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Star formation in Taurus Auriga Perseus and California nebulae

Part of: IAU Issue 315 - From Interstellar Clouds...

Published online by Cambridge University Press:  12 September 2016

L. Viktor Tóth ,
Sarolta Zahorecz ,
Gabor Marton ,
Yasuo Doi ,
Toshikazu Onishi  and
Kazuki Tokuda
L. Viktor Tóth
Affiliation:
Loránd Eötvös University, Pázmány P.s. 1/a, 1117 Budapest, Hungary
Sarolta Zahorecz
Affiliation:
Loránd Eötvös University, Pázmány P.s. 1/a, 1117 Budapest, Hungary ESO, Karl-Schwarzschild-Str. 2, D-85748 Garching bei München, Germany email: [email protected]
Gabor Marton
Affiliation:
Konkoly Observatory, H-1525 Budapest, PO Box 67, Hungary
Yasuo Doi
Affiliation:
University of Tokyo, 3-8-1 Komaba, Meguro-ku, Tokyo 153-8902, Japan
Toshikazu Onishi
Affiliation:
Osaka Prefecture University, 1-1 Gakuen-cho, Naka-ku, Sakai, Osaka 599-8531, Japan
Kazuki Tokuda
Affiliation:
Osaka Prefecture University, 1-1 Gakuen-cho, Naka-ku, Sakai, Osaka 599-8531, Japan
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Abstract

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Star formation and interstellar medium (ISM) structure were investigated in the Taurus, Auriga, Perseus and California (TAP) nearby star forming regions. Properties of the cold ISM was derived using AKARI FIR all sky maps, the Osaka-1.85m CO survey focusing to the all-sky Planck catalogue of Galactic Cold Clumps (PGCC). As many as 1041 infrared point sources were classified as young stellar object (YSO) based on multiband photometric data, and 384 of those are associated to a PGCC object. About 30% of the TAP PGCC clumps have associated YSOs.

Keywords

ISM: cloudsstars: formation
Type
Poster Papers
Information
Proceedings of the International Astronomical Union , Volume 11 , Symposium S315: From Interstellar Clouds to Star-Forming Galaxies: Universal Processes? , August 2015 , E75
Copyright
Copyright © International Astronomical Union 2016 

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