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Cambridge University Press (CUP), Proceedings of the International Astronomical Union, S315(11), 2015

DOI: 10.1017/s1743921316008371

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Star formation in Taurus Auriga Perseus and California nebulae

Journal article published in 2015 by L. Viktor Tóth, Sarolta Zahorecz, Gabor Marton ORCID, Yasuo Doi, Toshikazu Onishi, Kazuki Tokuda
This paper was not found in any repository, but could be made available legally by the author.
This paper was not found in any repository, but could be made available legally by the author.

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Abstract

AbstractStar 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.

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